National Library of Energy BETA

Sample records for mm mm mm

  1. mm,50 mm) and (90 mm,50 mm). There is an eight-unit cell separation between the two ports.

    E-Print Network [OSTI]

    Wai, Ping-kong Alexander

    mm,50 mm) and (90 mm,50 mm). There is an eight-unit cell separation between the two ports reported in Ref. 6. The calculated results are shown in Figure 4. The overall board height h 2.84 mm (112 mil), a 0.51 mm (20 mil), d 8.00 mm (315 mil), g 0.76 mm (30 mil), s 7.24 mm (285 mil), t1 2.36 mm (93

  2. mm-Wave Phase Shifters and Switches

    E-Print Network [OSTI]

    Adabi Firouzjaei, Ehsan

    2010-01-01

    combiners . . . . . . . . . . . 5.3 mm-Wave implementationfailed to predict current mm-wave design trend [1] . . . . .solutions . . . . . . . . mm-wave imaging for medical and

  3. DEFLECTION MEASUREMENTS OF 25 mm ALUMINUM COLLARS

    E-Print Network [OSTI]

    Peters, C.

    2010-01-01

    DEFLECTION MEASUREMENTS OF 25 mm ALUMINUM COLLARS· C. PetersDEFLECTION MEASUREMENTS OF 25 mm ALUMINUM COLLARS" C. Peters

  4. MISOSYS Disassembler -Disk version III DDDDD SSSSS MM MM BBBBB LL RRRRR

    E-Print Network [OSTI]

    Mann, Tim

    MISOSYS Disassembler - Disk version III DSMBLR - 1 DDDDD SSSSS MM MM BBBBB LL RRRRR DD DD SS SS MMM MMM BB BB LL RR RR DD DD SS MMMMMMM BB BB LL RR RR DD DD SSSSS MM M MM BBBBBB LL RRRRR DD DD SS MM MM BB BB LL RR RR DD DD SS SS MM MM BB BB LLLLLLL RR RR DDDDD SSSSS MM MM BBBBB LLLLLLL RR RR Copyright

  5. Discrimination Report ESTCP Project #MM-0437

    E-Print Network [OSTI]

    Gasperikova, Erika

    2008-01-01

    AS A FUNCTION OF TIME FOR 60 MM MORTAR . 23 F IGURE 12. PPOLARIZABILITY CURVES AS A FUNCTION OF TIME FOR 75 MM APAS A FUNCTION OF TIME FOR 81 MM MORTAR . 24 F IGURE 15. P

  6. mm-Wave Phase Shifters and Switches

    E-Print Network [OSTI]

    Adabi Firouzjaei, Ehsan

    2010-01-01

    4.1.1 Slow wave transmissioncombiners . . . . . . . . . . . 5.3 mm-Wave implementationfailed to predict current mm-wave design trend [1] . . . . .

  7. a 3.37 mm length b 3.32 mm diameter

    E-Print Network [OSTI]

    Marc, Robert E.

    5.2 ml retinal subtense 300 µm/deg retinal arc 51 mm retinal area* 1024 ± 184 mm2 total.3 µl retinal subtense 31 µm/deg retinal arc 4.9 mm retinal area 15.6 mm2 cone:rod ratio 0/deg retinal arc 10.6 mm retinal area 52 mm2 cone:rod ratio mean cone density* mm-2 mean rod

  8. Hickey -TT175, casts 220, line 222-229,231-232 Cruise cast lat(dd.mm.mm) lon(dd.mm.mm) Date/Time (MMDDYYHHMM) Total Scans

    E-Print Network [OSTI]

    Hickey, Barbara

    Hickey -TT175, casts 220, line 222- 229,231-232 Cruise cast lat(dd.mm.mm) lon(dd.mm.mm) Date,220 #12;Hickey -TT175, casts 220, line 222- 229,231-232 Cruise cast lat(dd.mm.mm) lon(dd.mm.mm) Date #12;Hickey -TT175, casts 220, line 222- 229,231-232 Cruise cast lat(dd.mm.mm) lon(dd.mm.mm) Date

  9. Hickey -TT174, casts 21, line 18 to cast 31, line 24 Cruise cast lat(dd.mm.mm) lon(dd.mm.mm) Date/Time (MMDDYYHHMM) Total Scans

    E-Print Network [OSTI]

    Hickey, Barbara

    Hickey -TT174, casts 21, line 18 to cast 31, line 24 Cruise cast lat(dd.mm.mm) lon(dd.mm.mm) Date;Hickey -TT174, casts 21, line 18 to cast 31, line 24 Cruise cast lat(dd.mm.mm) lon(dd.mm.mm) Date;Hickey -TT174, casts 21, line 18 to cast 31, line 24 Cruise cast lat(dd.mm.mm) lon(dd.mm.mm) Date

  10. Gash-Mm APP21¢¢¢§Q$ Cr

    E-Print Network [OSTI]

    Gash-Mm APP21¢¢¢§Q$ Cr. Partial Transfers by. Daniel Henry Gottliebl. The transfer for compact fibrations has been studied for some time now, [l,2,3,4,6,7,8,

  11. Demonstration Report: ESTCP UXO Discrimination Study ESTCP PROJECT # MM-0838

    E-Print Network [OSTI]

    Gasperikova, Erika

    2010-01-01

    Certification Program Project MM-0838. 7. REFERENCESSTUDY ESTCP PROJECT # MM-0838 SITE LOCATION: FORMER CAMP SANdesigned to detect UXO in the 20 mm to 155 mm size range for

  12. Brain Tissue Depth (mm) LightPowerDensity(mW/mm2

    E-Print Network [OSTI]

    Schnitzer, Mark

    Brain Tissue Depth (mm) LightPowerDensity(mW/mm2 ) Power Meter Tissue block Bare Fiber = 12° = 6 with the beveled cannula over CeA. d) Chart indicating estimated light power density seen at various distances from the fiber tip in mouse brain tissue when the light power density seen at the fiber tip was 7 mW (~99 mW/mm2

  13. direction. Three different pipette solutions were used: Cs-gluconate solution (150 mM CsOH, 5 mM CsCl, 135 mM sucrose, 10 mM HEPES, 1.5 mM EGTA and 1.5 mM EDTA

    E-Print Network [OSTI]

    Vale, Ronald D.

    direction. Three different pipette solutions were used: Cs-gluconate solution (150 mM CsOH, 5 mM CsCl, 135 mM sucrose, 10 mM HEPES, 1.5 mM EGTA and 1.5 mM EDTA (pH 7.2 with D-gluconic acid)); Na-gluconate solution (150 mM Na-gluconate, 5 mM NaCl, 135 mM sucrose, 10 mM HEPES, 1.5 mM EGTA and 1.5 mM EDTA (pH 7

  14. As of , , (yyyy,mm dd) Academic Title

    E-Print Network [OSTI]

    Yamamoto, Hirosuke

    ## As of , , (yyyy,mm dd) 1 2 3 / / yrs old 4 5 6 ) ) ) ) 7 8 dd dd 10 yyyy mm yyyy Academic Title yyyy mm mm mm Major Field Attach a sharp print taken within six months, City/Town, Country) Mobile Résumé Name Date of Birth (yyyy/mm/dd) Family Name E-mail Address Home

  15. Sub-mm Galaxies in Cosmological Simulations

    E-Print Network [OSTI]

    Mark A. Fardal; Neal Katz; David H. Weinberg; Romeel Davé; Lars Hernquist

    2001-07-16

    We study the predicted sub-mm emission from massive galaxies in a Lambda-CDM universe, using hydrodynamic cosmological simulations. Assuming that most of the emission from newly formed stars is absorbed and reradiated in the rest-frame far-IR, we calculate the number of galaxies that would be detected in sub-mm surveys conducted with SCUBA. The predicted number counts are strongly dependent on the assumed dust temperature and emissivity law. With plausible choices for SED parameters (e.g., T=35 K, beta=1.0), the simulation predictions reproduce the observed number counts above ~ 1 mJy. The sources have a broad redshift distribution with median z ~ 2, in reasonable agreement with observational constraints. However, the predicted count distribution may be too steep at the faint end, and the fraction of low redshift objects may be larger than observed. In this physical model of the sub-mm galaxy population, the objects detected in existing surveys consist mainly of massive galaxies (several M_*) forming stars fairly steadily over timescales ~ 10^8-10^9 years, at moderate rates ~100 Msun/yr. The typical descendants of these sub-mm sources are even more massive galaxies, with old stellar populations, found primarily in dense environments. While the resolution of our simulations is not sufficient to determine galaxy morphologies, these properties support the proposed identification of sub-mm sources with massive ellipticals in the process of formation. The most robust and distinctive prediction of this model, stemming directly from the long timescale and correspondingly moderate rate of star formation, is that the far-IR SEDs of SCUBA sources have a relative high 850 micron luminosity for a given bolometric luminosity. [Abridged

  16. QM/MM description of periodic systems

    E-Print Network [OSTI]

    Doll, K

    2015-01-01

    A QM/MM implementation for periodic systems is reported. This is done for the case of molecules and for systems with two and three-dimensional periodicity, which is suitable to model electrolytes in contact with electrodes. Tests on different water-containing systems, ranging from the water dimer up to liquid water indicate the correctness of the scheme. Furthermore, molecular dynamics simulations are performed, as a possible direction to study realistic systems.

  17. BBIIOOLLOOGGYY SSEEMMIINNAARR TTOO MM MM YY EEDD MM OO NN DD SS OO NN EENN DD OO WW EE DD LLEE CC TT UU RR EE

    E-Print Network [OSTI]

    Brown, Sally

    BBIIOOLLOOGGYY SSEEMMIINNAARR TTOO MM MM YY EEDD MM OO NN DD SS OO NN EENN DD OO WW EE DD LLEE CC TT UU RR EE 44::0000 PPMM SSEE MM II NNAA RR HHII TTCC HH CC OOCC KK HH AA LL LL 113322 RREE FF RR EE

  18. A 40 mm Bore Quadrupole Magnet for the SSC

    E-Print Network [OSTI]

    Taylor, C.E.

    2011-01-01

    No. DE-AC03-76SF00098. A 40 MM BORE QUADRUPOLE MAGNET FOR40mm 211 T/m+ 5.0m 1664 ( both rings) 6500A 0.648 mm9.78 mm 1.062/1.268 mm 1.2 deg. Coil bore diameter Gradient

  19. Coordinated mm/sub-mm observations of Sagittarius A* in May 2007

    E-Print Network [OSTI]

    D. Kunneriath; A. Eckart; S. Vogel; L. Sjouwerman; H. Wiesemeyer; R. Schoedel; F. K. Baganoff; M. Morris; T. Bertram; M. Dovciak; D. Downes; W. J. Duschl; V. Karas; S. Koenig; T. Krichbaum; M. Krips; R. -S. Lu; S. Markoff; J. Mauerhan; L. Meyer; J. Moultaka; K. Muzic; F. Najarro; K. Schuster; C. Straubmeier; C. Thum; G. Witzel; M. Zamaninasab; A. Zensus

    2008-10-01

    At the center of the Milky Way, with a distance of ~8 kpc, the compact source Sagittarius A* (SgrA*) can be associated with a super massive black hole of ~4x10^6 solar masses. SgrA* shows strong variability from the radio to the X-ray wavelength domains. Here we report on simultaneous NIR/sub-millimeter/X-ray observations from May 2007 that involved the NACO adaptive optics (AO) instrument at the European Southern Observatory's Very Large Telescope, the Australian Telescope Compact Array (ATCA), the US mm-array CARMA, the IRAM 30m mm-telescope, and other telescopes. We concentrate on the time series of mm/sub-mm data from CARMA, ATCA, and the MAMBO bolometer at the IRAM 30m telescope.

  20. Viewing the Evolution of Massive Star Formation through FIR/Sub-mm/mm Eyes

    E-Print Network [OSTI]

    Lihong Yao; E. R. Seaquist

    2006-05-25

    In this paper, we present an overview of our method of constructing a family of models for the far-infrared, sub-millimeter, and millimeter (FIR/sub-mm/mm) line emission of molecular and atomic gas surrounding massive star formation in starburst galaxies. We show the results of a case study, an expanding supershell centered around a massive star cluster with a particular set of input parameters and its application to nearby starburst galaxy M 82. This set of models can be used not only to interpret the observations of FIR/sub-mm/mm line emission from molecular and atomic gas, but also to investigate the physical environment and the initial cloud conditions in massive star forming regions as well as the ages of the starbursts through simulations for a wide range of input parameters. Finally, we discuss limitations of our models, and outline future work.

  1. Discrimination Report: ESTCP UXO Discrimination Study, ESTCP Project #MM-0437

    E-Print Network [OSTI]

    Gasperikova, Erika; Smith, J. Torquil; Morrison, H. Frank; Becker, Alex

    2007-01-01

    STUDY ESTCP PROJECT # MM-0437 Courtesy of Chris Gardner,POLARIZABILITIES , LOCATION AND ORIENTATION OF 81 MM M821A1POLARIZABILITIES , LOCATION AND ORIENTATION OF 105 MM M60

  2. DESIGN OF 15 mm COLLARS FOR SSC DIPOLE MAGNETS

    E-Print Network [OSTI]

    Peters, C.

    2010-01-01

    and Deflection for Five 15 mm S.S. Collar Types Welded 5.5.11. Collar Stiffness 15 mm 5.5. Collar Types Correlation ofMechanical measurement of 15 mm 5.5. collars used on eight

  3. 40 MM Grenade Launcher Qualification Requirements at Department...

    Office of Environmental Management (EM)

    40 MM Grenade Launcher Qualification Requirements at Department of Energy Sites, IG-0806 40 MM Grenade Launcher Qualification Requirements at Department of Energy Sites, IG-0806...

  4. Radio-mm-FIR Photometric Redshifts for (sub-)mm Galaxies

    E-Print Network [OSTI]

    Itziar Aretxaga; David H. Hughes; James S. Dunlop

    2007-02-20

    We present a comparison between the published optical, IR and CO spectroscopic redshifts of 86 (sub-)mm galaxies and their photometric redshifts as derived from long-wavelength radio-mm-FIR photometric data. The redshift accuracy measured for 13 sub-mm galaxies with at least one robustly determined colour in the radio-mm-FIR regime and additional constraining upper limits is z \\~0.3. This accuracy degrades to z~0.65 when only the 1.4GHz/850um spectral index is used, as derived from the analysis of a subsample of 58 galaxies with robustly determined redshifts. Despite the wide range of spectral energy distributions in the local galaxies that are used in an un-biased manner as templates, this analysis demonstrates that photometric redshifts can be effciently derived for sub-mm galaxies with a precision of Delta z < 0.5 using only the rest-frame FIR to radio wavelength data, suficient to guide the tuning of broad-band heterodyne observations (e.g. 100m GBT, 50m LMT, ALMA) or aid their determination in the case of a single line detection by these experiments.

  5. A 40 mm BORE Nb-Ti MODEL DIPOLE MAGNET

    E-Print Network [OSTI]

    Taylor, C.

    2010-01-01

    September 9-13, 1984 A 40 mm BORE Nb-Ti MODEL DIPOLE MAGNETNo. DE- AC03- 76SF0009B. A 40 mm BORE Nb- Tl MOOEL OIPOLEMPa) Midplane Shim (mm) ColI Length (mm) Number of Strands

  6. SUPPORTING INFORMATION METHODS Buffers. Buffer U is 20 mM TrisHCl, 6 mM NaCl, 1.7 mM MgCl2, 5 mM 2-mercaptoethanol (2-ME),

    E-Print Network [OSTI]

    Lohman, Timothy M.

    SUPPORTING INFORMATION METHODS Buffers. Buffer U is 20 mM Tris·HCl, 6 mM NaCl, 1.7 mM MgCl2, 5 mM 2H 7.5 at 25°C. SM buffer is 50 mM Tris·HCl, 0.1 M NaCl, 8 mM MgSO4, 0.01% gelatin, pH 7.5 at 25°C. Lysis buffer is 50 mM Tris·HCl, 0.2 M NaCl, 20% (w/v) sucrose, 15% (v/v) glycerol, 1 mM EDTA, 2 mM 2-ME

  7. Polarized mm And sub-mm Emission From Sgr A* At The Galactic Center

    E-Print Network [OSTI]

    Fulvio Melia; Siming Liu; Robert Coker

    2001-01-18

    The recent detection of significant linear polarization at mm and sub-mm wavelengths in the spectrum of Sgr A* (if confirmed) will be a useful probe of the conditions within several Schwarzschild radii ($r_S$) of the event horizon at the Galactic Center. Hydrodynamic simulations of gas flowing in the vicinity of this object suggest that the infalling gas circularizes when it approaches within $5-25 r_S$ of the black hole. We suggest that the sub-mm ``excess'' of emission seen in the spectrum of Sgr A* may be associated with radiation produced within the inner Keplerian region and that the observed polarization characteristics provide direct evidence for this phenomenon. The overall spectrum from this region, including the high-energy component due to bremsstrahlung and inverse Compton scattering processes, is at or below the recent {\\it Chandra} measurement, and may account for the X-ray source if it turns out to be the actual counterpart to Sgr A*.

  8. Digital Frequency Domain Multiplexer for mm-Wavelength Telescopes

    E-Print Network [OSTI]

    Dobbs, Matt

    2008-01-01

    for Large Scale Bolometer Arrays”, Monterey Far-IR, Sub-mmand mm Detector Technology Workshop proceedings, 2002, pp.Domain Multiplexer for mm-Wavelength Telescopes Matt Dobbs,

  9. MEASUREMENTS OF THE 1MM RECEIVER OPTICS Dick Plambeck

    E-Print Network [OSTI]

    MEASUREMENTS OF THE 1MM RECEIVER OPTICS Dick Plambeck Radio Astronomy laboratory, University of California, Berkeley, CA, 94720 March 2000 ABSTRACT When 1mm receivers were first installed on the BIMA of the 1mm receiver optics finally identified the problem -- two of the optical components in each dewar

  10. (Sub)mm Interferometry Applications in Star Formation Research

    E-Print Network [OSTI]

    Beuther, Henrik

    (Sub)mm Interferometry Applications in Star Formation Research H. Beuther1 Max-Planck Institute for Astronomy, K¨onigstuhl 17, 69117 Heidelberg, Germany beuther@mpia.de Abstract. Interferometry at (sub)mm structure e.g. details of accretion disks or molecular outflows and the sub(mm) wavelength bands

  11. A Tutorial on MM Algorithms David R. Hunter1

    E-Print Network [OSTI]

    Babu, G. Jogesh

    A Tutorial on MM Algorithms David R. Hunter1 Kenneth Lange2 Department of Statistics1 Penn State is a special case of the more general class of MM optimization algorithms, which typically exploit convexity rather than missing data in ma- jorizing or minorizing an objective function. In our opinion, MM

  12. Creating 35 mm Camera Active Pixel Sensors by Glenn Chapman*

    E-Print Network [OSTI]

    Chapman, Glenn H.

    #12;Creating 35 mm Camera Active Pixel Sensors by Glenn Chapman* and Yves Audet** * Simon Fraser Pixel Sensor imaging area device is studied which would be ideal for use with standard 35 mm cameras.5 per sq. cm. By being a retrofit for current 35 mm cameras, and having larger photodiode pixels than

  13. Summary of Decisions - MM DD YYYY - MM DD YYYY | Department of Energy

    Office of Energy Efficiency and Renewable Energy (EERE) Indexed Site

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Page on Delicious RankADVANCED MANUFACTURINGEnergyPlan | Department of Energy 1DepartmentS EM Pr7 -ofEnergy 9,7,3,MM DD

  14. Spectral Line Survey toward Young Massive Protostar NGC 2264 CMM3 in the 4 mm, 3 mm, and 0.8 mm Bands

    E-Print Network [OSTI]

    Watanabe, Yoshimasa; Lopez-Sepulcre, Ana; Furuya, Ryuta; Sakai, Takeshi; Hirota, Tomoya; Liu, Sheng-Yuan; Su, Yu-Nung; Yamamoto, Satoshi

    2015-01-01

    Spectral line survey observations are conducted toward the high-mass protostar candidate NGC 2264 CMM3 in the 4 mm, 3 mm, and 0.8 mm bands with the Nobeyama 45 m telescope and the Atacama Submillimeter Telescope Experiment (ASTE) 10 m telescope. In total, 265 emission lines are detected in the 4 mm and 3 mm bands, and 74 emission lines in the 0.8 mm band. As a result, 36 molecular species and 30 isotopologues are identified. In addition to the fundamental molecular species, many emission lines of carbon-chain molecules such as HC5N, C4H, CCS, and C3S are detected in the 4 mm and 3 mm bands. Deuterated molecular species are also detected with relatively strong intensities. On the other hand, emission lines of complex organic molecules such as HCOOCH3, and CH3OCH3 are found to be weak. For the molecules for which multiple transitions are detected, rotation temperatures are derived to be 7-33 K except for CH3OH. Emission lines with high upper-state energies (Eu > 150 K) are detected for CH3OH, indicating existen...

  15. A sub-mm imaging survey of ultracompact HII regions

    E-Print Network [OSTI]

    M. A. Thompson; J. Hatchell; G. H. Macdonald; T. J. Millar

    2001-12-19

    We present the preliminary results of a sub-mm imaging survey of ultracompact HII regions, conducted with the SCUBA bolometer array on JCMT.

  16. 663 900 1000 1100 1200 3514 Annual precipitation (mm)

    E-Print Network [OSTI]

    Beckage, Brian

    663 900 1000 1100 1200 3514 Annual precipitation (mm) -72.6 -71.5 -70.3 -69.2 -68.1 42 precipitation (mm) -72.6 -71.5 -70.3 -69.2 -68.1 42.143.144.245.346.4 Longitude (degree) Latitude(degree) (b) Baseline (1961-1990) 663 900 1000 1100 1200 3514 Annual precipitation (mm) -72.6 -71.5 -70.3 -69.2 -68.1 42

  17. The Innermost AGNs with Future mm-VLBI

    E-Print Network [OSTI]

    I. Agudo; T. P. Krichbaum; U. Bach; A. Pagels; B. W. Sohn; D. A. Graham; A. Witzel; J. A. Zensus; J. L. Gomez; M. Bremer; M. Grewing

    2005-10-31

    The capabilities of the Global mm-VLBI Array are summarized and demonstrated through actual images from our monitoring of extragalactic radio jets. This sensitive 3mm-VLBI interferometer is able to provide images of up to 50 microarcseconds resolution. For the near future, ALMA, the GBT, the LMT, CARMA, SRT, Yebes, Nobeyama and Noto are some of the most sensitive stations suitable to participate in mm-VLBI. This future array, together with the present Global mm-VLBI Array, would achieve 10 times better sensitivities than nowadays. Image fidelity would also largely increased. T he addition of ALMA would improve the (u,v)-coverage for sources with low declination (<20 deg.) and facilitate the VLBI imaging of the Galactic Centre source SgrA*.

  18. INTRODUCTION Pipunculidae are small (2-12 mm), inconspicuous

    E-Print Network [OSTI]

    Cotton, Sam

    INTRODUCTION Pipunculidae are small (2-12 mm), inconspicuous dark flies belonging. Humeri yellowish brown, mesonotum black with predominantly brown pollinosity. Femora yellow with dark, Hungary (foldvari@gmx.net) Keywords: faunistics, Tomosvaryella, Eudorylas #12;Eudorylas sp. Material

  19. (ISLiM) 2011 (2011.12.21-22) Platypus MM/CG

    E-Print Network [OSTI]

    Fukai, Tomoki

    #12;15 (ISLiM) 2011 (2011.12.21-22) 1 Platypus MM/CG 1982 3 1982 8 Cornell 1986 2 1988 4 1996 4 2001 4 2006 10 2011 4 HPCI #12;16 (ISLiM) 2011 (2011.12.21-22) 2 Platypus MM/CG 1. QM MM MM CG QM-MM-CG 3 QM MM QM/MM MM CG MM/CG 2. 2.1 ProteinDF QM DFT B3LYP 8,000 6 c 2.2 Platypus-QM/MM QM/MM QM MM QM/MM

  20. Galaxy formation & evolution: the far-ir/sub-mm view

    E-Print Network [OSTI]

    M. Cirasuolo; J. S. Dunlop

    2008-10-07

    We review our current knowledge of the population of high-redshift sub-mm/mm galaxies, with particular emphasis on recent results from the SCUBA HAlf Degree Extragalactic Survey (SHADES). All available evidence indicates that these objects form the high-redshift, high-luminosity, high-mass tail of the dusty starforming galaxy population revealed at lower redshifts and luminosities by Spitzer. Current theoretical models of galaxy formation struggle to reproduce these extreme objects in the numbers indicated by current surveys.

  1. 320 Herpetological Review 34(4), 2003 range = 17.028.7 mm; mean width = 11.6 mm, s = 0.73, range =

    E-Print Network [OSTI]

    Blouin-Demers, Gabriel

    320 Herpetological Review 34(4), 2003 range = 17.0­28.7 mm; mean width = 11.6 mm, s = 0.73, range = 10.5­12.5 mm). The third specimen collected in January is poorly preserved (IB 65538, 648 mm SVL, 150 mm TL) and had five oviductal eggs (mean length = 15.8 mm, s = 5.11, range = 10.0­ 22.2 mm; mean

  2. MM_swapImgRestore() { //v3.0 var i,x,a=document.MM_sr; for(i=0;a&&i

    E-Print Network [OSTI]

    MM_swapImgRestore() { //v3.0 var i,x,a=document.MM_sr; for(i=0;a&&i=a[i])&&x.oSrc;i++) x.src=x.oSrc; } function MM_preloadImages() { //v3.0 var d=document; if(d.images){ if(!d.MM_p) d.MM_p=new Array(); var i,j=d.MM_p.length,a=MM_preloadImages.arguments; for(i=0; i

  3. The Properties of Sub-mm Galaxies in Hierarchical Models

    E-Print Network [OSTI]

    Mark Swinbank; Cedric Lacey; Ian Smail; Carlton Baugh; Carlos Frenk; Andrew Blain; Scott Chapman; Kristen Coppin; Rob Ivison; Laura Hainline; Juan Gonzalez

    2008-09-11

    We use the combined GALFORM semi-analytical model of galaxy formation and GRASIL spectrophotometric code to investigate the properties of galaxies selected via their sub-mm emission. Our fiducial model has previously been shown to fit the properties of local ULIRGs, as well as the number counts of faint sub-mm galaxies. Here, we test the model in detail by comparing the SEDs and stellar, dynamical, gas and halo masses of sub-mm galaxies against observational data. We precisely mimic the sub-mm and radio selection function of the observations and show that the predicted far-infrared properties of model galaxies with S_850>5mJy and S_1.4>30uJy are in good agreement with observations. Although the dust emission model does not assume a single dust temperature, the far-infrared SEDs are well described by single component modified black-body spectrum with characteristic temperature 32+/-5K. We also find evidence that the observations may have uncovered evolution in the far-infrared--radio relation in ULIRGs out to z~2. We show that the predicted redshift distribution of sub-mm galaxies provides a reasonable fit to the observational data with a median redshift z=2.0, with the radio-selected subset predicted to make up approximately 75% of the population. However, the predicted K-band and mid-infrared (3--8um) flux densities of the sub-mm galaxies (and LBGs) are up to a factor 10x fainter than observed. This discrepancy may indicate that the stellar masses of the sub-mm galaxies in the model are too low: M~10^10Mo, while observations suggest more massive systems, M~10^11Mo. Finally, we discuss the potential modifications to the models which may improve the fit to the observational data. [Abridged

  4. Starburst Models For FIR/sub-mm/mm Line Emission. I. An Expanding Supershell Surrounding A Massive Star Cluster

    E-Print Network [OSTI]

    Lihong Yao; T. A. Bell; S. Viti; J. A. Yates; E. R. Seaquist

    2005-09-19

    The effect of a newly born star cluster inside a giant molecular cloud (GMC) is to produce a hot bubble and a thin, dense shell of interstellar gas and dust swept up by the H II expansion, strong stellar winds, and repeated supernova explosions. Lying at the inner side of the shell is the photodissociation region (PDR), the origin of much of the far-infrared/sub-millimeter/millimeter (FIR/sub-mm/mm) radiation from the interstellar medium (ISM). We present a model for the expanding shell at different stages of its expansion which predict mm/sub-mm and far-IR emission line intensities from a series of key molecular and atomic constituents in the shell. The kinematic properties of the swept-up shell predicted by our model are in very good agreement with the measurements of the supershell detected in the nearby starburst galaxy M 82. We compare the modeling results with the ratio-ratio plots of the FIR/sub-mm/mm line emission in the central 1.0 kpc region to investigate the mechanism of star forming activity in M 82. Our model has yielded appropriate gas densities, temperatures, and structure scales compared to those measured in M 82, and the total H2 content is compatible with the observations. This implies that the neutral ISM of the central star-forming region is a product of fragments of the evolving shells.

  5. Discrimination Report: A Multisensor system for detection and characterization of UXO, ESTCP Project MM-0437,

    E-Print Network [OSTI]

    Gasperikova, Erika; Smith, J. Torquil; Morrison, H.Frank; Becker, Alex

    2008-01-01

    characterization of UXO (MM-0437) - Demonstration report:AND CHARACTERIZATION OF UXO MM-0437 SITE LOCATION: U.S. ARMYcharacterization of UXO (MM-0437) - Demonstration report,

  6. Quadruply Bonded Dimetal Units Supported by 2,4,6-Triisopropylbenzoates MM(TiPB)4 (MM ) Mo2, MoW, and W2)

    E-Print Network [OSTI]

    Turro, Claudia

    Quadruply Bonded Dimetal Units Supported by 2,4,6-Triisopropylbenzoates MM(TiPB)4 (MM ) Mo2, Mo, and cyclic voltammetry) of the new compounds MM(TiPB)4, where MM ) MoW and W2 and TiPB ) 2 in the visible region of the spectrum that are assigned to MM to arylcarboxylate * transitions, 1 MLCT. Each

  7. (Sub-)mm interferometry in massive star-forming regions

    E-Print Network [OSTI]

    H. Beuther

    2003-08-21

    (Sub-)mm interferometry is the most favorable technique to investigate the earliest stages of massive star formation. I will outline general applications in that field and discuss results of different sub-topics (hot core chemistry and massive molecular outflows). Furthermore, recent data obtained with the Submillimeter Array will be shown to present the unique capabilities of this new instrument. Finally, I will give a short outlook on the main physical topics of massive star formation to be tackled with (sub-)mm interferometry within the next decade.

  8. Powering mm-Size Wireless Implants for Brain-Machine Interfaces

    E-Print Network [OSTI]

    Mark, Michael

    2011-01-01

    4 Proof-of-Concept: A 1 mm 3 Neural Transponder Linkfor power transfer to a 1 x 1 mm 2 implanted antenna withantenna with a diameter of 15 mm and a 1 mm 2 implant

  9. Hickey -TT174, casts 1 to cast 11 Cruise cast lat (dd.mm.m) lon(dd.mm.m) Date/Time (MMDDYYHHMM) Total Scan

    E-Print Network [OSTI]

    Hickey, Barbara

    Hickey -TT174, casts 1 to cast 11 Cruise cast lat (dd.mm.m) lon(dd.mm.m) Date/Time (MMDDYYHHMM;Hickey -TT174, casts 1 to cast 11 Cruise cast lat (dd.mm.m) lon(dd.mm.m) Date/Time (MMDDYYHHMM) Total -TT174, casts 1 to cast 11 Cruise cast lat (dd.mm.m) lon(dd.mm.m) Date/Time (MMDDYYHHMM) Total Scan

  10. Ferrite-Cored Solenoidal Induction Coil Sensor for BUD (MM-1667)

    E-Print Network [OSTI]

    Morrison, F.

    2012-01-01

    Research and Development Program Project MM-1667.INDUCTION COIL SENSOR FOR BUD (MM-1667) Frank Morrison 1 ,

  11. 3 mm Anisotropy Measurement: On the Quadrupole Component in the Cosmic Background Radiation

    E-Print Network [OSTI]

    Lubin, Philip M.; Epstein, Gerald L.; Smoot, George F.

    1982-01-01

    Mixer Impedance transformer 3 mm local oscillator X m 4°K -Frequency (GHz) I Wavelength (mm) XBL SOUTH CELESTIAL POLE

  12. The simultaneous spectrum of Sgr A* from 20cm to 1mm and the nature of the mm-excess

    E-Print Network [OSTI]

    Heino Falcke; W. M. Goss; Hiroshi Matsuo; Peter Teuben; Jun-Hui Zhao; Robert Zylka

    1998-01-12

    We report results from a multiwavelength campaign to measure the simultaneous spectrum of the super-massive black hole candidate Sgr A* in the Galactic Center from cm to mm-wavelengths using the VLA, BIMA, the Nobeyama 45m, and the IRAM 30m telescopes. The observations confirm that the previously detected mm-excess is an intrinsic feature of the spectrum of Sgr A*. The excess can be interpreted as due to the presence of an ultra-compact component of relativistic plasma with a size of a few Schwarzschild radii near the black hole. If so, Sgr A* might offer the unique possibility to image the putative black hole against the background of this component with future mm-VLBI experiments.

  13. Course Outline Engineer 2MM3 Electrical Circuits & Power

    E-Print Network [OSTI]

    Haykin, Simon

    .ece.mcmaster.ca/~mrhowlader/2mm3/notes.htm Text Book: S.J. Chapman, Electric Machinery Fundamentals, McGraw Hill, Fifth Edition Course Description: Fundamentals of electromechanical energy conversion. Motors and generators. Fundamentals of Magnetic Circuits; 2. Fundamentals of Electrical Circuits, Phasors; 3. Power in AC Circuits; 4

  14. Mm/submm observations of symbiotic binary stars

    E-Print Network [OSTI]

    J. Mikolajewska; R. J. Ivison; A. Omont

    2002-10-22

    We present and discuss mm/submm observations of quiescent S-type symbiotic systems, and compare them with popular models proposed to account for their radio emission. We find that the M giant mass-loss rates derived from our observations are systematically higher than those reported for single M giants.

  15. FISHERY STATISTICS I OF THE UNITED STATESmmmMM

    E-Print Network [OSTI]

    ^^ FISHERY STATISTICS I OF THE UNITED STATESmmmMM 'f^ gjIP^Ws^WI'l STATISTICAL DIGEST NO. 25 Fish Statistical Digest 25 FISHERY STATISTICS OF THE UNITED STATES 1949 BY A. W. ANDERSON and C. E. PETERSON UNITED. Government Printing Office, Washington 25, D. C. - - - Price $1.25 (paper) #12;Fishery Statistics

  16. In-vehicle mm-Wave Channel Model and Measurement

    E-Print Network [OSTI]

    Zemen, Thomas

    . I. INTRODUCTION The ever increasing vehicle efficiency goes hand in hand with weight savings. OneIn-vehicle mm-Wave Channel Model and Measurement Jiri Blumenstein, Tomas Mikulasek, Roman Marsalek measurements carried out in the intra­ vehicle environment. Channels in the millimeter-wave (MMW) frequency

  17. Hans Peter Schwefel Wireless Networks III, Fall 2005: MM1, IP Mobility Support

    E-Print Network [OSTI]

    Schwefel, Hans-Peter

    Page 1 Hans Peter Schwefel Wireless Networks III, Fall 2005: MM1, IP Mobility Support Wireless@kom.auc.dk http://www.kom.auc.dk/~hps http://www.kom.auc.dk/~tatiana · Mm1 IP Mobility Support (HPS) · Mm2 Wireless TCP (HPS) · Mm3 Wireless applications, SIP & IMS (HPS) · Mm4 Ad-hoc Networks I (TKM) · Mm5 Ad

  18. Sub-mm clues to elliptical galaxy formation

    E-Print Network [OSTI]

    James S. Dunlop

    2000-11-03

    There is growing evidence that, at the S(850) mm galaxy population (and hence a potentially significant fraction of the sub-mm background) is associated with the star-forming Lyman-break population already detected at optical wavelengths. However, the implied star-formation rates in such objects (typically 3-30 solar masses per year) fall one or two orders of magnitude short of the level of star-forming activity required to produce the most massive elliptical galaxies on a timescale ~ 1 Gyr. If a significant fraction of massive ellipticals did form the bulk of their stars in short-lived massive starbursts at high redshift, then they should presumably be found among the brighter, S(850) ~ 10 mJy sub-mm sources which are undoubtedly not part of the Lyman-break population. A first powerful clue that this is indeed the case comes from our major SCUBA survey of radio galaxies, which indicates that massive dust-enshrouded star-formation in at least this subset of massive ellipticals is largely confined to z > 2.5, with a mean redshift z = 3.5. While radio selection raises concerns about bias, I argue that our current knowledge of the brightest (S(850) ~ 10 mJy) sub-mm sources detected in unbiased SCUBA imaging surveys indicates that they are also largely confined to this same high-z regime. Consequently, while the most recent number counts imply such extreme sources can contribute only 5-10% of the sub-mm background, their comoving number density (in the redshift band 3 < z < 5) is 1-2 x 10^{-5} per cubic megaparsec, sufficient to account for the formation of all ellipticals of comparable mass to radio galaxies (~4L-star) in the present-day universe.

  19. Taiwan geology Plate collision at 80 mm/yr

    E-Print Network [OSTI]

    Gung, Yuancheng

    4 #12;Meander #12;#12;#12;=/ #12;: () () () () () : : 2.0 1.51.75 1.25 1.0 #12/yr (Ratio: 1.9%, Area: 0.024%) Average sediment discharge to ocean: 384 Mt/yr --- 160 Mt/yr (544 Mt.m.s) = Sediments (ton.s-1) Sediments (ton.s-1) ÷ Density (t/m3) ÷ Area (m2) = Erosion (mm.s-1) Calculation: Stream

  20. VLBA Imaging at 7 mm and Linear Polarimetric Observations at 6 cm and 3 mm of Sagittarius A*

    E-Print Network [OSTI]

    Geoffrey C. Bower; Heino Falcke; Don Backer; Melvyn Wright

    1998-11-13

    We summarize the results of 7 mm VLBA imaging of Sgr A* and discuss some of the difficulties of accurately constraining the size of Sgr A* with VLBI observations. Our imaging results are fully consistent with the hypothesis that the VLBA image of Sgr A* is a resolved elliptical Gaussian caused by the scattering of an intervening thermal plasma. We show that determination of the minor axis size at 7 mm with the VLBA is very unreliable. We also present new polarimetric observations from the VLA and from the BIMA array of Sgr A*. At 4.8 GHz, we find an upper limit to the polarization of 0.1%. At 86 GHz, we report a marginal detection of $1 \\pm 1$% linear polarization. We discuss the effects of interstellar propagation on the linear polarization and consider the significance of very low intrinsic linear polarization in Sgr A*.

  1. What we need to return at the telescope New array at 1mm with better sensitvity

    E-Print Network [OSTI]

    Leclercq, Samuel

    What we need to return at the telescope New array at 1mm with better sensitvity Magnetic field pixels with 3 preamplifiers (1 at 2mm and 2 at 1mm) · 300 pixels at 2mm · 600 pixels at 1mm Automatic

  2. SUB-MM-WAVE TECHNOLOGIES: SYSTEMS, ICS, THZ TRANSISTORS M. J. W. Rodwell

    E-Print Network [OSTI]

    Rodwell, Mark J. W.

    SUB-MM-WAVE TECHNOLOGIES: SYSTEMS, ICS, THZ TRANSISTORS M. J. W. Rodwell Department of Electrical Engineering University of California, Santa Barbara, CA 93105 Abstract mm-wave and sub-mm-wave outdoor, bipolar transistors, mm- waves, sub-mm-waves, THz. I. INTRODUCTION With progressive scaling of junction

  3. Hans Peter Schwefel Wireless Networks III, Fall 2005: MM2, Wireless TCP

    E-Print Network [OSTI]

    Schwefel, Hans-Peter

    Page 1 Hans Peter Schwefel Wireless Networks III, Fall 2005: MM2, Wireless TCP Wireless Networks Wireless TCP (HPS) · Mm3 Wireless applications, SIP & IMS (HPS) · Mm4 Ad-hoc Networks I (TKM) · Mm5 Ad Schwefel Wireless Networks III, Fall 2005: MM2, Wireless TCP Background: IP Protocol Stack Network Layer

  4. Pulling of 3 mm diameter AlSb rods by micro-pulling down method

    E-Print Network [OSTI]

    Bourret-Courchesne Ph.D., Edith

    2009-01-01

    SUBCONTRACT #6836278 Pulling of 3 mm diameter AlSb rods by1 cm long, and at least 3 mm in diameter. provided by LBNL.l Crucible Power/T° Speed (mm/min) Seed Results Crucible

  5. Ab initio simulations of two-dimensional electronic spectra: The SOS//QM/MM approach

    E-Print Network [OSTI]

    Rivalta, I; Nenov, A; Cerullo, G; Mukamel, S; Garavelli, M; Garavelli, M

    2013-01-01

    working on hybrid QM/MM molecular dynamics simulations. InElectronic Spectra: The SOS//QM/MM Approach Ivan Rivalta,* [molecular mechanics (QM/MM) scheme and the sum-over-states (

  6. Fabrication and Test of TQS01 - a 90 mm Nb3Sn Quadrupole Magnet for LARP

    E-Print Network [OSTI]

    Dietderich, D.

    2008-01-01

    and Test of TQS01 – a 90 mm Nb 3 Sn Quadrupole Magnet forTQS and TQC) with a 90-mm aperture are being constructed atStructure for an LHC 90 mm Nb 3 Sn quadrupole magnet”, IEEE

  7. Atherosclerotic Plaque Characterization by 0.5-mm-Slice Multislice Computed Tomographic Imaging

    E-Print Network [OSTI]

    2007-01-01

    PIaque Characterization by O.5-mm- SIice Multislice ComputedIt has been proposed that O.5-mm-slice multislice computedperformed to compare the O.5-mm-slice ultrasound findings.

  8. DESIGN AND CONSTRUCTION OF A 15 T, 120 MM BORE IR QUADRUPOLE MAGNET FOR LARP

    E-Print Network [OSTI]

    Caspi, S.

    2011-01-01

    is developing a large bore (120 mm) IR quadrupole ( H Q )quadrupole ( H Q ) that extends the bore size from 90 mm to120 mm and pushes the field at the conductor just over 15 T.

  9. MECHANICAL TEST RESULTS ON DIPOLE MODEL C-l 25 mm ALUMINUM COLLARS

    E-Print Network [OSTI]

    Peters, C.

    2010-01-01

    RESULTS ON DIPOLE MODEL C-1 25 mm ALUMINUM COLLARS C. PetersRESULTS ON DIPOLE MODEL C-I 25 mm ALUMINUM COLLARS· CraigON DIPOLE MODEL C-I 25 mm ALUMINUM COLLARS Craig Peters

  10. High-efficiency 5000 lines/mm multilayer-coated blazed grating for EUV wavelengths

    E-Print Network [OSTI]

    Voronov, Dmitriy

    2010-01-01

    High-efficiency 5000 lines/mm multilayer-coated blazedthat show, for a 5000 l/mm grating diffracting in the 3 rdof 12.5 nm with a 1000 groove/mm grating [7]. A denser 2400

  11. A multisensor system for detection and characterization of UXO (MM-0437) - Demonstration Report

    E-Print Network [OSTI]

    Gasperikova, Erika; Smith, J.T.; Morrison, H.F.; Becker, A.

    2006-01-01

    AND CHARACTERIZATION OF UXO MM-0437 SITE LOCATION: U.S. ARMYwas designed to detect and characterize UXO in the 20 mm to155 mm size range for depths between 0 and 1 m. The

  12. Fabrication and Test of TQS01 -- a 90 mm Nb3Sn Quadrupole Magnet for LARP

    E-Print Network [OSTI]

    Caspi, S.

    2008-01-01

    and Test of TQS01 – a 90 mm Nb 3 Sn Quadrupole Magnet forTQS and TQC) with a 90-mm aperture are being constructed atStructure for an LHC 90 mm Nb 3 Sn quadrupole magnet”, IEEE

  13. A Multisensor system for the detection and characterization of UXO MM-0437

    E-Print Network [OSTI]

    Gasperikova, Erika; Becker, A.; Morrison, H.F.; Smith, J.T.

    2006-01-01

    AND CHARACTERIZATION OF UXO MM-0437 SITE LOCATION: U.S. ARMYwas designed to detect and characterize UXO in the 20 mm to155 mm size range for depths between 0 and 1 m. The

  14. Design of HD2: a 15 T Nb3Sn dipole with a 35 mm bore

    E-Print Network [OSTI]

    Sabbi, G.

    2009-01-01

    a 15 Tesla Nb 3 Sn Dipole with a 35 mm Bore G. Sabbi, S.E.dipole field above 15 T, a 35 mm bore, and nominal fieldstainless steel tube, providing a 35 mm diameter clear bore.

  15. Solar ALMA: Observation-Based Simulations of the mm and sub-mm Emissions from Active Regions

    E-Print Network [OSTI]

    Fleishman, Gregory; Nita, Gelu

    2015-01-01

    We developed an efficient algorithm integrated in our 3D modeling tool, GX Simulator (Nita et al. 2015), allowing quick computation of the synthetic intensity and polarization maps of solar active regions (AR) in the ALMA spectral range. The algorithm analyzes the photospheric input (white light and magnetogram) to classify a given photospheric pixel to belong to a given photospheric structure. Then, a 1D chromospheric model (Fontenla et al. 2009) is added on top of each pixel, which forms a chromospheric model of the AR. Next step is computation of the mm and sub-mm emission produced from this chromosphere model. A huge advantage of this approach is that emission from any given AR can be synthesized very fast, on the order of a few minutes after the AR selection. Using the GX Simulator tool it is also possible to produce synthetic maps of the microwave (gyroresonance) and EUV emission from the same AR model and compare them with the ALMA synthetic maps and with the corresponding observed microwave and/or EUV...

  16. Length: 4-15 mm Larvae (maggots): Creamy-white to green or

    E-Print Network [OSTI]

    Isaacs, Rufus

    Hover fly Syrphidae Length: 4-15 mm Larvae (maggots): Creamy-white to green or brown. Worm flies" or "flower flies"). Eggs: Small (1 mm in length). Cylindrical, white and laid singly on leaves or shoots near aphid colonies. 15 mm4 mm #12;Pupae: Green, tan or brown. Typically pear- shaped with a pair

  17. Oct. 12, 2005 QM/MM: What have we learned, where are we, and where

    E-Print Network [OSTI]

    Truhlar, Donald G

    1 Oct. 12, 2005 QM/MM: What have we learned, where are we, and where do we go from here? Hai Lin1/molecular mechanical (QM/MM) calculations, including their advantages and disadvantages. There is a special emphasis tests of QM/MM methods and summarize what we learn about QM/MM from these studies. We also discuss some

  18. Steering with Eyes Closed: mm-Wave Beam Steering without In-Band Measurement

    E-Print Network [OSTI]

    Knightly, Edward W.

    Steering with Eyes Closed: mm-Wave Beam Steering without In-Band Measurement Thomas Nitsche that removes in-band overhead for directional mm-Wave link establishment. Our sys- tem architecture couples mm-Wave and legacy 2.4/5 GHz bands using out-of-band direction inference to establish (overhead-free) multi-Gbps mm

  19. SSC 50 mm dipole magnet cryostat thermal measurement results

    SciTech Connect (OSTI)

    Boroski, W.N.; Nicol, T.H.; Ruschman, M.K.; Schoo, C.J.

    1993-05-01

    A prototype Superconducting Super Collider (SSC) 50 mm dipole magnet cryostat, DCA323, was instrumented at Fermilab and delivered to the SSC Laboratory for installation into the accelerator systems string test facility. In series with other magnets, the instrumented cryostat will be used to quantify and verify cryostat thermal performance with respect to design requirements. Prior to leaving Fermilab, DCA323 was subjected to magnetic testing at the Magnet Test Facility (MTF). This presented an opportunity to obtain preliminary thermal performance data under simulated operating conditions. It should be noted that measurements of overall cryostat thermal performance were not possible during the MTF measurements as the magnet test stands are designed for magnetic rather than thermal testing. They are not designed to limit heat inleak to the ends of the cryostat, which has been shown to have a significant effect on overall measured thermal performance. Nonetheless, these measurements do offer insight into the performance of several of the cryostat components and sub-systems.

  20. Elsevier AMS Ch19-N53138 Job code: CPC 5-2-2007 4:45p.m. Page:441 Trimsize:165240MM Basal Fonts:Times Margins:Top:13MM Gutter:20MM Font Size:10/12pt Text Width:125MM Depth:47 Lines

    E-Print Network [OSTI]

    Jones, William D.

    .m. Page:441 Trimsize:165×240MM Basal Fonts:Times Margins:Top:13MM Gutter:20MM Font Size:10/12pt Text Width:125MM Depth:47 Lines CHAPTER 19 Perspective and prospects for pincer ligand chemistry William D. Jones 45 46 47 Elsevier AMS Ch19-N53138 Job code: CPC 5-2-2007 4:45p.m. Page:442 Trimsize:165×240MM Basal

  1. MM + MSE Student Initiated Dual Degree Information Pg. 1 of 4 Master of Management (Ross School of Business)

    E-Print Network [OSTI]

    Awtar, Shorya

    MM + MSE Student Initiated Dual Degree Information Pg. 1 of 4 Master of Management (Ross School Normal MM Program Requirements 24.75cr MM Business Core + 6cr MM Business Electives = 30.75cr MM Core(s): 6 Credits + #12;MM + MSE Student Initiated Dual Degree Information Pg. 2 of 4 MM Boot Camp

  2. GPS interseismic periods interseismic slip rate deficit 23.6 mm/yr 294

    E-Print Network [OSTI]

    Chen, Wen-Shan

    interseismic slip rate deficit 23.6 mm/yr 294° 21.6-27.7 mm/y lock 8-12 700 0.65 3.4 26.4 mm/yr 285 Kuochen et al., 2004 40 km1991-2002ML3 19831992 2000 1983 1974 16-23°30 mm/yrChen et al., 199119141979 Biq, 198411° Yu et al., 199028.5±3.0mm/yr 353-1°2004-2006GPS 30°19.3 mm/yr 300° 1954 #12

  3. Sub-mm Jet Properties of the X-Ray Binary Swift J1745$-$26

    E-Print Network [OSTI]

    Tetarenko, A J; Miller-Jones, J C A; Curran, P A; Russell, T D; Coulson, I M; Heinz, S; Maitra, D; Markoff, S B; Migliari, S; Petitpas, G R; Rupen, M P; Rushton, A P; Russell, D M; Sarazin, C L

    2015-01-01

    We present the results of our observations of the early stages of the 2012--2013 outburst of the transient black hole X-ray binary (BHXRB), Swift J1745$-$26, with the VLA, SMA, and JCMT (SCUBA--2). Our data mark the first multiple-band mm & sub-mm observations of a BHXRB. During our observations the system was in the hard accretion state producing a steady, compact jet. The unique combination of radio and mm/sub-mm data allows us to directly measure the spectral indices in and between the radio and mm/sub-mm regimes, including the first mm/sub-mm spectral index measured for a BHXRB. Spectral fitting revealed that both the mm (230 GHz) and sub-mm (350 GHz) measurements are consistent with extrapolations of an inverted power-law from contemporaneous radio data (1--30 GHz). This indicates that, as standard jet models predict, a power-law extending up to mm/sub-mm frequencies can adequately describe the spectrum, and suggests that the mechanism driving spectral inversion could be responsible for the high mm/s...

  4. National Conference on Mechanisms and Machines (NaCoMM07), IISc, Bangalore, India, December 12-13, 2007 NaCoMM-2007-60

    E-Print Network [OSTI]

    Saha, Subir Kumar

    ). Rotational input is provided to the crankshaft of the machine by a flexible coupling connected to an electric13th National Conference on Mechanisms and Machines (NaCoMM07), IISc, Bangalore, India, December 12-13, 2007 NaCoMM-2007-60 Synthesis and Analysis of a New Mechanism for Sheep Shearing Machine Vineet

  5. Heat Transfer -2 A pure platinum wire with diameter D = 3 mm and length L = 20 mm is placed outside on a day when air temperature

    E-Print Network [OSTI]

    Virginia Tech

    Heat Transfer - 2 A pure platinum wire with diameter D = 3 mm and length L = 20 mm is placed outside on a day when air temperature T = 10o C. The heat transfer coefficient at the wire's surface h equation that includes all heat transfer mechanisms involved in this problem. Write this energy balance

  6. A Polarizable QM/MM Explicit Solvent Model for Computational Electrochemistry in Water

    E-Print Network [OSTI]

    Wang, Lee-Ping

    We present a quantum mechanical/molecular mechanical (QM/MM) explicit solvent model for the computation of standard reduction potentials E[subscript 0]. The QM/MM model uses density functional theory (DFT) to model the ...

  7. Ultraviolet Spectroscopy of Protein Backbone Transitions in Aqueous Solution: Combined QM and MM Simulations

    E-Print Network [OSTI]

    Mukamel, Shaul

    Ultraviolet Spectroscopy of Protein Backbone Transitions in Aqueous Solution: Combined QM and MM (MM) calculations is developed to simulate the n f * and f * backbone transitions of proteins using a new algorithm, EHEF, which combines a molecular dynamics (MD) trajectory obtained with a MM

  8. Design of HD2: a 15 T Nb3Sn dipole with a 35 mm bore

    E-Print Network [OSTI]

    Sabbi, G.

    2009-01-01

    Nb 3 Sn Dipole with a 35 mm Bore G. Sabbi, S.E. Bartlett, S.T Copper current density kA/ mm 2 Inductance mH/m Storedminimum winding radius of 12.5 mm. There are 28 turns in the

  9. Geometry Optimization with QM/MM, ONIOM, and Other Combined Methods. I. Microiterations

    E-Print Network [OSTI]

    Schlegel, H. Bernhard

    Geometry Optimization with QM/MM, ONIOM, and Other Combined Methods. I. Microiterations Abstract: Hybrid energy methods such as QM/MM and ONIOM, that combine different levels of theory into one of theory and the larger, remaining region treated by an inexpensive method such as molecular mechanics (MM

  10. DESIGN AND PERFORMANCE OF 40 mm, 6.5 T, COLLARED, COLD-IRON MODEL MAGNETS

    E-Print Network [OSTI]

    Peters, C.

    2010-01-01

    DESIGN AND PERFORMANCE OF 40 MM, 6.5 T, COLLARED, COLD-IRONAND P,E RFORMANCE OF 40 MM, 6.5 T, COLLARED, COLD-IRON MODELmagnet winding is 1.574 inches (40 mm), which is the same as

  11. Breakdown of 2mm symmetry in electron diffraction from multiwalled carbon nanotubes

    E-Print Network [OSTI]

    Qin, Lu-Chang

    Breakdown of 2mm symmetry in electron diffraction from multiwalled carbon nanotubes Zejian Liu of single-walled carbon nanotubes always have 2mm symmetry regardless if the nanotubes them- selves have such symmetry. We here show that, for the case of multiwalled carbon nanotubes, the 2mm symmetry can break down

  12. HEAT TRANSFER THROUGH He II IN A 9.6 m LONG 35 mm ID TUBE

    E-Print Network [OSTI]

    Caspi, S.

    2010-01-01

    He II IN A 9.6 m LONG 35 mm ID TUBE S. Caspi and R.V.He II IN A 9.6 m LONG 35 mm ID TUBE* S. Caspi and R. V.He II IN A 9.6 m LONG 35 mm 10 TUBE S. Caspi and R. V.

  13. BBIIOOLLOOGGYY SSEEMMIINNAARR PPRR OO MM OO TT II OO NN LLEE CC TT UU RR EE

    E-Print Network [OSTI]

    Brown, Sally

    BBIIOOLLOOGGYY SSEEMMIINNAARR PPRR OO MM OO TT II OO NN LLEE CC TT UU RR EE 44::0000 PPMM SSEE MM II NNAA RR PPHH YY SSII CCSS //AASS TTRR OONN OO MM YY AAUU DD .. AA110022 RREE FF RR EE SSHHMM EE NN

  14. The 69-mm forsterite band as a dust temperature indicator J. E. Bowey,1P

    E-Print Network [OSTI]

    Bowey, Janet

    The 69-mm forsterite band as a dust temperature indicator J. E. Bowey,1P M. J. Barlow,1 F. J) occurs at 69.67 mm at room temperature (295 K); for olivines with *10 per cent Fe the corresponding feature is at *73 mm. The Mg-rich forsterite feature is observed in a variety of ISO LWS spectra

  15. A 10,000 groove/mm multilayer coated grating for EUV spectroscopy

    E-Print Network [OSTI]

    Voronov, Dmytro

    2011-01-01

    a groove density of 5000 lines/mm using a process based ongroove density of 10,000 lines/mm, and coated it with an Al/groove density of 10,000 lines/mm (a); 3D AFM images of the

  16. MM5 Contrail Forecasting in Alaska Martin Stuefer, Xiande Meng and Gerd Wendler

    E-Print Network [OSTI]

    Stuefer, Martin

    MM5 Contrail Forecasting in Alaska Martin Stuefer, Xiande Meng and Gerd Wendler Geophysical Institute, University of Alaska, Fairbanks 1. Abstract Fifth-generation mesoscale model (MM5) is being used air. Algorithm input data are MM5 forecasted temperature and humidity values at defined pressure

  17. Fragment-Based QM/MM Method for Modeling Molecular Crystals and Clusters

    E-Print Network [OSTI]

    Nanda, Kaushik

    2013-01-01

    of Molecular Crystals With a Fragment-Based QM/MM Method 5.1Theory: A Fragment-Based QM/MM Study 6.1 Outline . . . . .off from the QM PES to the MM PES due to the spatial damping

  18. Measurements of the Cosmic Background Radiation Temperature at 3.3 and 9.1 MM

    E-Print Network [OSTI]

    Witebsky, C.; De Amici, G.; Smoot, G.F.; Friedman, S.D.

    1983-01-01

    TEMPERATURE- AT 3.3 AND 9.1 MM C. Witebsky, G. De Amici, andTEMPERATURE AT 3.3 AND 9.1 MM Chris Witebsky, Giovanni Decharacteristics of the 3.3 and 9.1 mm radiometers Wavelength

  19. HEAT TRANSFER THROUGH He II IN A 9.6 m LONG 35 mm ID TUBE

    E-Print Network [OSTI]

    Caspi, S.

    2010-01-01

    THROUGH He II IN A 9.6 m LONG 35 mm ID TUBE S. Caspi andTHROUGH He II IN A 9.6 m LONG 35 mm ID TUBE* S. Caspi and R.THROUGH He II IN A 9.6 m LONG 35 mm 10 TUBE S. Caspi and R.

  20. Supporting Information for Mixed Quantum Mechanical/Molecular Mechanical (QM/MM) Study

    E-Print Network [OSTI]

    Gherman, Benjamin F.

    S1 Supporting Information for Mixed Quantum Mechanical/Molecular Mechanical (QM/MM) Study geometries for the QM/MM-optimized R61 acyl-enzyme intermediate protonation/hydrogen bond configurations-blue, O-red, H-gray, S-yellow. (1) (2a) #12;S3 (3) #12;S4 Figure S2. Active site geometries for the QM/MM

  1. QM/MM methods for crystalline defects. Part 2: Consistent energy and force-mixing

    E-Print Network [OSTI]

    Chen, Huajie

    2015-01-01

    QM/MM hybrid methods employ accurate quantum (QM) models only in regions of interest (defects) and switch to computationally cheaper interatomic potential (MM) models to describe the crystalline bulk. We develop two QM/MM hybrid methods for crystalline defect simulations, an energy-based and a force-based formulation, employing a tight binding QM model. Both methods build on two principles: (i) locality of the QM model; and (ii) constructing the MM model as an explicit and controllable approximation of the QM model. This approach enables us to establish explicit convergence rates in terms of the size of QM region.

  2. Progresses in Ab Initio QM/MM Free Energy Simulations of Electrostatic Energies in Proteins: Accelerated QM/MM Studies of pKa, Redox Reactions and Solvation Free Energies

    E-Print Network [OSTI]

    Kamerlin, Shina C. L.

    2009-01-01

    J. ; Glennon, T. ; Warshel, A. QM/MM approaches for studyingProgresses in Ab Initio QM/MM Free Energy Simulations ofin Proteins: Accelerated QM/MM Studies of pK a , Redox

  3. Fabrication and characterization of a 0.5-mm lutetium oxyorthosilicate detector array for high-resolution PET applications

    E-Print Network [OSTI]

    Stickel, Jennifer R; Qi, Jinyi; Cherry, Simon R

    2007-01-01

    2006;51:2131–2142. 0.5- MM LSO A RRAY FOR PET • Stickel etand Characterization of a 0.5-mm Lutetium Oxyorthosilicatelicate (LSO) arrays with 0.5-mm pixels was coupled to

  4. MM versus ML estimates of structural equation models with interaction terms: robustness to non-normality of the consistency property

    E-Print Network [OSTI]

    Mooijaart, Ab; Satorra, Albert

    2011-01-01

    of-?t summaries for the MM method degrees of freedom chi-regarding the robustness of the MM method to non-normality.MM versus ML estimates of structural equation models with

  5. Development of TQC01, a 90 mm Nb3 Sn Model Quadrupole for LHC Upgrade Based on SS Collar

    E-Print Network [OSTI]

    Bossert, R. C.

    2009-01-01

    Development of TQC01, a 90 mm Nb 3 Sn Model Quadrupole foriron yoke laminations and 12 mm thick stainless steel skinsby ap- proximately 10 MPa per mm of key depth. During the

  6. Water Management EC Kumbur and MM Mench, The Pennsylvania State University, University Park, PA, USA

    E-Print Network [OSTI]

    Mench, Matthew M.

    , and molten carbonate fuel cell have been, or continue to be, developed. However, ubiquitous integration a schematic of a typical PEMFC assembly. In a PEMFC, the electrolyte (15­180 mm thick) is a flexible polymer- ported on larger carbon particles (B45­90 mm diameter). The fuel (typically hydrogen (H2)) and oxidizer

  7. Mountain Lion 'MmJUN7-r946 WQDOS HOLE, MASS

    E-Print Network [OSTI]

    mm ^m' ''AzM. Mountain Lion 'MmJUN7-r946 WQDOS HOLE, MASS CIRCULAR 6 FISH AND WILDLIFE SERVICE U. S For sale by the Superintendent of Documents Washinston 25, D. C. : Price 5 cents #12;MOUNTAIN LION TRAPPING Service nPHE AMERICAN MOUNTAIN LION (Felis concolor) is one of J- the largest predatory animals

  8. Evaluation of Offshore Wind Simulations with MM5 in the Japanese and Danish Coastal Waters

    E-Print Network [OSTI]

    Heinemann, Detlev

    Evaluation of Offshore Wind Simulations with MM5 in the Japanese and Danish Coastal Waters Teruo to evaluate the accuracy of offshore wind simulation with the mesoscale model MM5, long-term simulations to simulate offshore wind conditions in the Japanese coastal waters even using a mesoscale model, compared

  9. Hybrid QM/MM Car-Parrinello Simulations of Catalytic and Enzymatic Reactions

    E-Print Network [OSTI]

    Guidoni, Leonardo

    1 Hybrid QM/MM Car-Parrinello Simulations of Catalytic and Enzymatic Reactions MariaCarola Colombo, we review some recent applications of hybrid Car-Parrinello simulations of chemical and biological recently developed a combination of these two techniques into a hybrid QM/MM Car-Parrinello scheme [4

  10. Chemical Vapor Deposition Growth of 5 mm Hexagonal Single-Crystal Graphene from Ethanol

    E-Print Network [OSTI]

    Maruyama, Shigeo

    Chemical Vapor Deposition Growth of 5 mm Hexagonal Single-Crystal Graphene from Ethanol Xiao Chen1 as large as 5 mm can be synthesized from ethanol via chemical vapor deposition (CVD). Key conditions for the successful reduction in nucleation density are extremely low partial pressure of ethanol vapor and pre

  11. Condensation heat transfer characteristics of R410A-oil mixture in 5 mm and 4 mm outside diameter horizontal microfin tubes

    SciTech Connect (OSTI)

    Huang, Xiangchao; Ding, Guoliang; Hu, Haitao; Zhu, Yu. [Institute of Refrigeration and Cryogenics, Shanghai Jiaotong University, Shanghai 200240 (China); Gao, Yifeng [International Copper Association Shanghai Office, Shanghai 200020 (China); Deng, Bin [Institute of Heat Transfer Technology, Golden Dragon Precise Copper Tube Group Inc., Shanghai 200135 (China)

    2010-10-15

    Condensation heat transfer characteristics of R410A-oil mixture in 5 mm and 4 mm outside diameter horizontal microfin tubes were investigated experimentally. The experimental condensing temperature is 40 C, and nominal oil concentration range is from 0% to 5%. The test results indicate that the presence of oil deteriorates the heat transfer. The deterioration effect is negligible at nominal oil concentration of 1%, and becomes obvious with the increase of nominal oil concentration. At 5% nominal oil concentration, the heat transfer coefficient of R410A-oil mixture is found to have a maximum reduction of 25.1% and 23.8% for 5 mm and 4 mm tubes, respectively. The predictabilities of the existing condensation heat transfer correlations were verified with the experimental data, and Yu and Koyama correlation shows the best predictability. By replacing the pure refrigerant properties with the mixture's properties, Yu and Koyama correlation has a deviation of -15% to + 20% in predicting the local condensation heat transfer coefficient of R410A-oil mixture. (author)

  12. Convergence in the QM-Only and QM/MM Modeling of Enzymatic Reactions: A Case Study for Acetylene

    E-Print Network [OSTI]

    Liao, Rongzhen

    Convergence in the QM-Only and QM/MM Modeling of Enzymatic Reactions: A Case Study for Acetylene/molecular mechanics (MM) calculations on an enzyme- catalyzed reaction to assess the convergence behavior of QM- only and QM/MM energies with respect to the size of the cho- sen QM region. The QM and MM parts are described

  13. Comparison of QM-Only and QM/MM Models for the Mechanism of Tungsten-Dependent Acetylene Hydratase

    E-Print Network [OSTI]

    Liao, Rongzhen

    Comparison of QM-Only and QM/MM Models for the Mechanism of Tungsten-Dependent Acetylene Hydratase-only and QM/MM approaches for the modeling of enzymatic reactions. For this purpose, we present a QM/MM case of the previously suggested one-water attack mechanism. The QM/MM calculations with the minimal QM region M1 (32

  14. 1. The derivative of y = mm“ at x = 2. A bacteria culture starts with ...

    E-Print Network [OSTI]

    The derivative of y = mm“ at x = 2. A bacteria culture starts with 200 bacteria and grows at a rate proportional to its size. After 2 hours there were 400 bacteria.

  15. Simulating the high-redshift universe in the sub-mm

    E-Print Network [OSTI]

    Eelco van Kampen

    2003-10-10

    I present various simulations of an on-going large sub-mm survey, SHADES, showing how constraints can be put on galaxy formation models and cosmology from this survey.

  16. Artist's rendition of a 1.54 mm-emitting laser

    E-Print Network [OSTI]

    Sargent, Edward H. "Ted"

    Artist's rendition of a 1.54 mm-emitting laser made by solution- processing a colloidal quantum dot detectivity, represented by the symbol D*. Epitaxially grown InGaAs devices on an InP substrate achieve

  17. Power supply switching for a mm-wave asymmetric multilevel outphasing power amplifier system

    E-Print Network [OSTI]

    Spaulding, Jonathon David

    2010-01-01

    This thesis demonstrates power switches to be used in our new Asymmetric Multilevel Outphasing (AMO) transmitter architecture at mm-wave frequencies. The AMO topology breaks the linearity vs. efficiency design objective ...

  18. Can the supermassive objects at the centers of galaxies be traversable wormholes? The first test of strong gravity for mm/sub-mm VLBI facilities

    E-Print Network [OSTI]

    Cosimo Bambi

    2013-04-29

    The near future mm/sub-mm VLBI experiments are ambitious projects aiming at imaging the "shadow" of the supermassive black hole candidate at the center of the Milky Way and of the ones in nearby galaxies. An accurate observation of the shape of the shadow can potentially test the nature of these objects and verify if they are Kerr black holes, as predicted by general relativity. However, previous work on the subject has shown that the shadows produced in other spacetimes are very similar to the one of the Kerr background, suggesting that tests of strong gravity are not really possible with these facilities in the near future. In this work, I instead point out that it will be relatively easy to distinguish black holes from wormholes, topologically non-trivial structures of the spacetime that might have been formed in the early Universe and might connect our Universe with other universes.

  19. On the cross-correlation of sub-mm sources and optically-selected galaxies

    E-Print Network [OSTI]

    Chris Blake; Alexandra Pope; Douglas Scott; Bahram Mobasher

    2006-02-20

    Bright sub-mm galaxies are expected to arise in massive highly-biased haloes, and hence exhibit strong clustering. We argue that a valuable tool for measuring these clustering properties is the cross-correlation of sub-mm galaxies with faint optically-selected sources. We analyze populations of SCUBA-detected and optical galaxies in the GOODS-N survey area. Using optical/IR photometric-redshift information, we search for correlations induced by two separate effects: (1) cosmic magnification of background sub-mm sources by foreground dark matter haloes traced by optical galaxies at lower redshifts; and (2) galaxy clustering due to sub-mm and optical sources tracing the same population of haloes where their redshift distributions overlap. Regarding cosmic magnification, we find no detectable correlation. Our null result is consistent with a theoretical model for the cosmic magnification, and we show that a dramatic increase in the number of sub-mm sources will be required to measure the effect reliably. Regarding clustering, we find evidence at the 3.5-sigma level for a cross-correlation between sub-mm and optical galaxies analyzed in identical photometric redshift slices. The data hint that the sub-mm sources have an enhanced bias parameter compared to the optically-selected population (with a significance of 2-sigma). The next generation of deep sub-mm surveys can potentially perform an accurate measurement of each of these cross-correlations, adding a new set of diagnostics for understanding the development of massive structure in the Universe.

  20. The local sub-mm luminosity functions and predictions from ASTRO-F/SIRTF to Herschel

    E-Print Network [OSTI]

    Stephen Serjeant; Diana Harrison

    2003-09-23

    We present new determinations of the local sub-mm luminosity functions. We find the local sub-mm luminosity density converging to 7.3+/-0.2 x 10^19 W/Hz/Mpc^3 /h_65 at 850um solving the ``sub-mm Olbers' Paradox.'' Using the sub-mm colour temperature relations from the SCUBA Local Universe Galaxy Survey, and the discovery of excess 450um excess emission in these galaxies, we interpolate and extrapolate the IRAS detections to make predictions of the SEDs of all 15411 PSC-z galaxies from 50-3000um. Despite the long extrapolations we find excellent agreement with (a) the 90um luminosity function of Serjeant et al. (2001), (b) the 850um luminosity function of Dunne et al. (2000), (c) the mm-wave photometry of Andreani & Franceschini (1996); (d) the asymptotic differential and integral source count predictions at 50-3000um by Rowan-Robinson (2001). Remarkably, the local luminosity density and the extragalactic background light together strongly constrain the cosmic star formation history for a wide class of evolutionary assumptions. We find that the extragalactic background light, the 850um 8mJy source counts, and the Omega_* constraints all independently point to a decline in the comoving star formation rate at z>1.

  1. A spectral line survey in the 2 mm and 1.3 mm windows toward the carbon rich envelope of IRC +10216

    E-Print Network [OSTI]

    J. H. He; Dinh-V-Trung; S. Kwok; H. S. P. Mueller; Y. Zhang; T. Hasegawa; T. C. Peng; Y. C. Huang

    2008-04-14

    We present the results of our spectral line surveys in the 2 mm and 1.3 mm windows toward the carbon rich envelope of IRC +10216. Totally 377 lines are detected, among which 360 lines are assigned to 57 known molecules (including 29 rare isotopomers and 2 cyclic isomers). Only 17 weak lines remain unidentified. Rotational lines of isotopomers 13CCH and HN13C are detected for the first time in IRC +10216. The detection of the formaldehyde lines in this star is also confirmed. Possible abundance difference among the three 13C substituted isotopic isomers of HC3N is reported. Isotopic ratios of C and O are confirmed to be non-solar while those of S and Si to be nearly solar. Column densities have been estimated for 15 molecular species. Modified spectroscopic parameters have been calculated for NaCN, Na13CN, KCN and SiC2. Transition frequencies from the present observations were used to improve the spectroscopic parameters of Si13CC, 29SiC2 and 30SiC2.

  2. High Heat Flux Exposure Tests on 10mm Beryllium Tiles Brazed on Actively Cooled Vapotron made from CUCRZR

    E-Print Network [OSTI]

    High Heat Flux Exposure Tests on 10mm Beryllium Tiles Brazed on Actively Cooled Vapotron made from CUCRZR

  3. MM5 Aids Forecasters Over the past five years a group in the Atmospheric

    E-Print Network [OSTI]

    Doty, Sharon Lafferty

    Jaeglé's specialty is atmospheric chemistry. Her research deals with analysis and modelingMM5 Aids Forecasters Over the past five years a group in the Atmospheric Sciences department has around the region. (see Page 8) New Faculty Join Atmospheric Sciences In the past year, Atmospheric

  4. ENGINEER 2MM3 -Electrical Circuits & Power TERM 1, 2014/15

    E-Print Network [OSTI]

    Haykin, Simon

    Machinery Fundamentals, McGraw Hill, Fourth Edition, 2005. Reference Book: T. Wildi, Electrical machines of electric circuits, phasors 3. Transformers 4. AC generators and motors 5. Three-phase circuits 7. 3-phaseENGINEER 2MM3 - Electrical Circuits & Power TERM 1, 2014/15 Course Outline Instructor: Shiva

  5. Sub-mm imaging of a proto-cluster region at z=3.09

    E-Print Network [OSTI]

    S. C. Chapman; G. F. Lewis; D. Scott; E. Richards; C. Borys; C. C. Steidel; K. L. Adelberger; A. E. Shapley

    2000-10-04

    We have used the Submillimetre Common-User Bolometer Array (SCUBA) detector on the James Clerk Maxwell Telescope (JCMT) to measure bright sub-mm emission associated with a recently discovered extensive (>100/h kpc) and highly luminous, `blob' of Ly-alpha emission at z=3.09. The blob lies within a known large overdensity of optical sources in the z=3.07-3.11 range, and is centered on a locally overdense peak within this region. The best explanation for the copious sub-mm emission is a dust obscured continuum source, which may produce the ionizing flux for the Ly-alpha cloud. Cooling gas explanations are plausible but excessively complicated, and the 450/850 micron ratio rules out a significant fraction of the signal arising from the Sunyaev-Zel'dovich increment. At least two additional ~10 mJy sub-mm detections in the SCUBA map, with a surface density significantly higher than in blank field surveys, suggests that they may be associated with the z=3.09 structure. A SCUBA `photometry' observation of a second nearby Ly-alpha blob tentatively detects a weaker sub-mm counterpart.

  6. Interferometric detections of GOODS 850-5 at 1 mm and 1.4 GHz

    E-Print Network [OSTI]

    H. Dannerbauer; F. Walter; G. Morrison

    2007-12-19

    We have obtained a position (at sub-arcsecond accuracy) of the submillimeter bright source GOODS 850-5 (also known as GN10) in the GOODS North field using the IRAM Plateau de Bure interferometer at 1.25 mm wavelengths (MM J123633+6214.1, flux density: S(1.25 mm)=5.0+-1.0 mJy). This source has no optical counterpart in deep ACS imaging down to a limiting magnitude of i(775)=28.4 mag and its position is coincident with the position found in recent sub-millimeter mapping obtained at the SMA (Wang et al. 2007). Using deep VLA imaging at 20 cm, we find a radio source (S(20 cm)=32.7+-4.3 microJy) at the same position that is significantly brighter than reported in Wang et al. The source is detected by Spitzer in IRAC as well as at 24 microns. We apply different photometric redshift estimators using measurements of the dusty, mid/far-infrared part of the SED and derive a redshift z~4. Given our detection in the millimeter and radio we consider a significantly higher redshift (e.g., z~6 Wang et al. 2007) unlikely. MM J123633+6214.1 alias GOODS 850-5 nevertheless constitutes a bright representative of the high-redshift tail of the submillimeter galaxy population that may contribute a significant fraction to the (sub)millimeter background.

  7. Using 50-mm electrostatic membrane deformable mirror in astronomical adaptive optics

    E-Print Network [OSTI]

    Tokovinin, Andrei A.

    achievable modulation of the local radius of curvature of the mirror is ±25 m. Simulations of the AO system with 37 electrodes (hereafter DM-37) is used in the AO system at McMath-Pierce solar telescope2 telescope.4 A larger number of actuators is needed, so we select a DM with 79 electrodes and 50-mm membrane

  8. Press Advertising 39x3col (390mm x 3 cols)

    E-Print Network [OSTI]

    Press Advertising 39x3col (390mm x 3 cols) Total cost of ad Canberra Times $1,682.49 HES $4. 200 words Canberra Times $1,037.29 HES $2,785.00 STANDALONE Press advertising describes job advertisements in a printed medium such as newspapers, magazines and journals. We currently primarily advertised

  9. Formaldehyde around 3.5 and 5.7-mm: Measurement and calculation of broadening coefficients

    E-Print Network [OSTI]

    Gamache, Robert R.

    Formaldehyde around 3.5 and 5.7-mm: Measurement and calculation of broadening coefficients D February 2010 Keywords: Formaldehyde Broadening coefficients Widths H2CO Fourier transform spectroscopy has been generated to complete the whole HITRAN 2008 version of formaldehyde (available

  10. High-Resolution Regional Climate Simulations over Iceland Using Polar MM5* DAVID H. BROMWICH

    E-Print Network [OSTI]

    Howat, Ian M.

    High-Resolution Regional Climate Simulations over Iceland Using Polar MM5* DAVID H. BROMWICH Polar, Environmental and Food Agency, Reykjavik, Iceland (Manuscript received 9 August 2004, in final form 23 June 2005) ABSTRACT High-resolution regional climate simulations of Iceland for 1991­2000 have been performed using

  11. THE JOURNAL OF CHEMICAL PHYSICS 139, 244108 (2013) Periodic boundary conditions for QM/MM calculations: Ewald summation

    E-Print Network [OSTI]

    Herbert, John

    2013-01-01

    THE JOURNAL OF CHEMICAL PHYSICS 139, 244108 (2013) Periodic boundary conditions for QM/MM of Ewald summation for use in mixed quantum mechanics/molecular mechanics (QM/MM) calculations is presented a method for applying PBC to mixed quantum mechanics/molecular mechanics (QM/MM) simula- tions. We

  12. Reflective Cracking Study: First-level Report on HVS Testing on Section 587RF - 45 mm RAC-G Overlay

    E-Print Network [OSTI]

    Wu, R; Jones, David; Harvey, John T

    2008-01-01

    Testing on Section 589RF — 45 mm MB4-G Overlay (UCPRC-RR-Testing on Section 587RF — 45 mm RAC-G Overlay (UCPRC-RR-Testing on Section 588RF — 90 mm AR4000-D Overlay (UCPRC-RR-

  13. ASSEMBLY AND TEST OF A 120 MM BORE 15 T NB3SN QUADRUPOLE FOR THE LHC UPGRADE

    E-Print Network [OSTI]

    Felice, H.

    2011-01-01

    ASSEMBLY AND TEST OF A 120 MM BORE 15 T NB SN QUADRUPOLE FORdeveloping a 1-meter long, 120 mm bore N b S n IR quadrupoleH Q is a 1-meter long 120 mm aperture cos29 quadrupole. The

  14. Mechanical Design of HD2, a 15 T Nb3Sn Dipole Magnet with a 35 mm Bore

    E-Print Network [OSTI]

    Ferracin, P.

    2008-01-01

    T Nb 3 Sn Dipole Magnet with a 35 mm Bore P. Ferracin, S. E.a 15 T Nb 3 Sn Dipole with a 35 mm Bore”, IEEE Trans. Appl.design uses 51 strands of 0.8 mm diameter. With respect to

  15. Reflective Cracking Study: First-level Report on HVS Testing on Section 586RF - 45 mm MB15-GOverlay

    E-Print Network [OSTI]

    Jones, David; Wu, R; Harvey, John T

    2008-01-01

    Testing on Section 590RF — 90 mm MB4-G Overlay (UCPRC-RR-Testing on Section 589RF — 45 mm MB4-G Overlay (UCPRC-RR-Testing on Section 587RF — 45 mm RAC-G Overlay (UCPRC-RR-

  16. Assembly and Test of HD2, a 36 mm bore high field Nb3Sn Dipole Magnet

    E-Print Network [OSTI]

    Ferracin, P.

    2010-01-01

    Assembly and Test of HD2, a 36 mm bore high field Nb 3 Sna 15 T Nb 3 Sn dipole with a 35 mm bore”, IEEE Trans. Appl.Nb 3 Sn dipole magnet with a 35 mm bore”, IEEE Trans. Appl.

  17. Reflective Cracking Study: First-Level Report on HVS Testing on Section 589RF - 45 mm MB4-G Overlay

    E-Print Network [OSTI]

    Jones, David; Harvey, John T; Wu, R; Lea, J.

    2008-01-01

    Testing on Section 590RF — 90 mm MB4-G Overlay (UCPRC-RR-Testing on Section 589RF — 45 mm MB4-G Overlay (UCPRC-RR-Testing on Section 587RF — 45 mm RAC-G Overlay (UCPRC-RR-

  18. Wyko Optical Profiler This machine investigates variations in topography for surfaces ranging from very smooth to 2mm step

    E-Print Network [OSTI]

    ranging from very smooth to 2mm step height. Basic interferometric principles are used with light. Range Vertical Resolution PSI up to 150 nm 3 VSI up to 2mm 3 nm Operation 1. Power up: · Log In · Power sample, lower objectives to a position that is approximately 1mm above sample. Closely watch all

  19. Reflective Cracking Study: First-Level Report on HVS Testing on Section 590RF - 90 mm MB4-G Overlay

    E-Print Network [OSTI]

    Jones, David; Tsai, Bor-Wen; Harvey, John T

    2008-01-01

    Testing on Section 587RF — 45 mm RAC-G Overlay (UCPRC-RR-Testing on Section 588RF — 90 mm AR4000-D Overlay (UCPRC-RR-Testing on Section 586RF — 45 mm MB15-G Overlay (UCPRC-RR-

  20. Test Results of HD2, A High Field Nb3Sn Dipole with A 36 MM Bore

    E-Print Network [OSTI]

    Ferracin, Paolo

    2010-01-01

    a 15 T Nb 3 Sn dipole with a 35 mm bore”, IEEE Trans. Appl.Nb 3 Sn dipole magnet with a 35 mm bore”, IEEE Trans. Appl.NB 3 SN DIPOLE WITH A 36 MM BORE * P. Ferracin # , LBNL,

  1. Reflective Cracking Study: First-level Report on HVS Testing on Section 588RF - 90 mm AR4000-DOverlay

    E-Print Network [OSTI]

    Jones, David; Wu, R; Harvey, John T

    2008-01-01

    Testing on Section 590RF — 90 mm MB4-G Overlay (UCPRC-RR-Testing on Section 589RF — 45 mm MB4-G Overlay (UCPRC-RR-Testing on Section 587RF — 45 mm RAC-G Overlay (UCPRC-RR-

  2. Mechanical Design of HD2, a 15 T Nb3Sn Dipole Magnet with a 35 mm Bore

    E-Print Network [OSTI]

    Ferracin, P.

    2008-01-01

    T Nb 3 Sn Dipole Magnet with a 35 mm Bore P. Ferracin, S. E.a 15 T Nb 3 Sn Dipole with a 35 mm Bore”, IEEE Trans. Appl.a dipole field above 15 T, a 35 mm clear bore, and nominal

  3. Radio, Sub-mm, and X-ray Studies of Gamma-Ray Burst Host Galaxies

    E-Print Network [OSTI]

    E. Berger

    2001-12-29

    The study of gamma-ray burst (GRB) host galaxies in the radio, sub-mm, and X-ray wavelength regimes began only recently, in contrast to optical studies. This is mainly due to the long timescale on which the radio afterglow emission decays, and to the intrinsic faintness of radio emission from star-forming galaxies at z~1, as well as source confusion in sub-mm observations; X-ray observations of GRB hosts have simply not been attempted yet. Despite these difficulties, we have recently made the first detections of radio and sub-mm emission from the host galaxies of GRB980703 and GRB010222, respectively, using the VLA and the SCUBA instrument on JCMT. In both cases we find that the inferred star formation rates (~500 solar masses per year) and bolometric luminosities (~few 10^12 solar luminosities) indicate that these galaxies are possibly analogous to the local population of Ultra-Luminous Infrared Galaxies (ULIRGs) undergoing a starburst. However, there is a modest probability that the observed emission is due to AGN activity rather than star formation, thus requiring observations with Chandra or XMM. The sample of GRB hosts offers a number of unique advantages to the broader question of the evolution of galaxies and star formation from high redshift to the present time since: (i) GRBs trace massive stars, (ii) are detectable to high redshifts, and (iii) have immense dust penetrating power. Therefore, radio/sub-mm/X-ray observations of GRB hosts can potentially provide crucial information both on the nature of the GRB host galaxies, and on the history of star formation.

  4. Performance of HQ02, an optimized version of the 120 mm $Nb_3Sn$ LARP quadrupole

    E-Print Network [OSTI]

    Chlachidze, G; Anerella, M; Borgnolutti, F; Bossert, R; Caspi, S; Cheng, D W; Dietderich, D; Felice, H; Ferracin, P; Ghosh, A; Godeke, A; Hafalia A R; Marchevsky, M; Orris, D; Roy, P K; Sabbi, G L; Salmi, T; Schmalzle, J; Sylvester, C; Tartaglia, M; Tompkins, J; Wanderer, P; Wang, X R; Zlobin, A V

    2013-01-01

    In preparation for the high luminosity upgrade of the Large Hadron Collider (LHC), the LHC Accelerator Research Program (LARP) is developing a new generation of large aperture high-field quadrupoles based on Nb3Sn technology. One meter long and 120 mm diameter HQ quadrupoles are currently produced as a step toward the eventual aperture of 150 mm. Tests of the first series of HQ coils revealed the necessity for further optimization of the coil design and fabrication process. A new model (HQ02) has been fabricated with several design modifications, including a reduction of the cable size and an improved insulation scheme. Coils in this magnet are made of a cored cable using 0.778 mm diameter Nb3Sn strands of RRP 108/127 sub-element design. The HQ02 magnet has been fabricated at LBNL and BNL, and then tested at Fermilab. This paper summarizes the performance of HQ02 at 4.5 K and 1.9 K temperatures.

  5. The Contribution of Faint Blue Galaxies to the Sub-mm Counts and Background

    E-Print Network [OSTI]

    Geoff S. Busswell; Tom Shanks

    2000-10-24

    Observations in the submillimetre waveband have recently revealed a new population of luminous, sub-mm sources. These are proposed to lie at high redshift and to be optically faint due to their high intrinsic dust obscuration. The presence of dust has been previously invoked in optical galaxy count models which assume $\\tau=9$ Gyr Bruzual & Charlot evolution for spirals and these fit the count data well from U to K. We now show that by using either a 1/$\\lambda$ or Calzetti absorption law for the dust and re-distributing the evolved spiral galaxy UV radiation into the far infra-red(FIR), these models can account for all of the `faint'($\\leq1$mJy) $850\\mu$m galaxy counts, but fail to fit 'bright'($\\ge2$mJy) sources, indicating that another explanation for the sub-mm counts may apply at brighter fluxes(e.g. QSOs, ULIRGs). We find that the main contribution to the faint, sub-mm number counts is in the redshift range $0.5 < z < 3$, peaking at $z\\approx 1.8$. The above model, using either dust law, can also explain a significant proportion of the extra-galactic background at $850\\mu$m as well as producing a reasonable fit to the bright $60\\mu m$ IRAS counts.

  6. Fabrication and characterization of a 0.5-mm lutetium oxyorthosilicate detector array for high-resolution PET applications

    E-Print Network [OSTI]

    Stickel, Jennifer R; Qi, Jinyi; Cherry, Simon R

    2007-01-01

    and Characterization of a 0.5-mm Lutetium OxyorthosilicateIn this work, a pair of lutetium oxyorthosi- licate (LSO)PET; high spatial resolution; lutetium oxyorthosilicate;

  7. Self-consistent QM/MM methodologies for structural refinement of photosystem II and other macromolecules of biological interest

    SciTech Connect (OSTI)

    Batista, Enrique R [Los Alamos National Laboratory; Sproviero, Eduardo M [YALE UNIV; Newcomer, Michael [YALE UNIV; Gascon, Jose A [YALE UNIV; Batista, Victor S [YALE UNIV

    2008-01-01

    The combination of quantum mechanics and molecular mechanics (QM/MM) is one of the most promising approaches to study the structure, function, and properties of proteins and nucleic acids. However, there some instances in which the limitations of either the MM (lack of a proper electronic description) or QM (limited to a few number of atoms) methods prevent a proper description of the system. To address this issue, we review here our approach to fine-tune the structure of biological systems using post-QM/MM refinements. These protocols are based on spectroscopy data, and/or partitioning of the system to extend the QM description to a larger region of a protein. We illustrate these methodologies through applications to several biomolecules, which were pre-optimized at the QM/MM level and then further refined using postQM/MM refinement methodologies: mod(QM/MM), which refines the atomic charges of the residues included in the MM region accounting for polarization effects; mod(QM/MM)-opt that partition the MM region in smaller parts and optimizes each part in an iterative. self-consistent way, and the Polarized-Extended X-Ray Absorption Fine Structure (P-EXAFS) fitting procedure, which fine-tune the atomic coordinates to reproduce experimental polarized EXAFS spectra. The first two techniques were applied to the guanine quadruplex. while the P-EXAFS refinement was applied to the oxygen evolving complex of photosystem II.

  8. An experiment to detect gravity at sub-mm scale with high-Q mechanical oscillators

    E-Print Network [OSTI]

    L. Haiberger; M. Weingran; H. Wenz; S. Schiller

    2005-10-20

    Silicon double paddle oscillators are well suited for the detection of weak forces because of their high Q factor (about 10^5 at room temperature). We describe an experiment aimed at the detection of gravitational forces between masses at sub-mm distance using such an oscillator. Gravitational excitation is produced by a rotating aluminium disk with platinum segments. The force sensitivity of this apparatus is about 10 fN at room temperature for 1000 s averaging time at room temperature. The current limitations to detection of the gravitational force are mentioned.

  9. Sub-mm tests of the gravitational inverse-square law

    E-Print Network [OSTI]

    E. G. Adelberger

    2002-02-02

    Sub-mm tests of the gravitational inverse-square law are interesting from several quite different perspectives. This paper discusses work by the Eot-Wash group performed since the publication of our initial result in February 2001. We find no evidence for short-range Yukawa interactions. Our results provide an upper limit of 200 micrometers on the size of the largest ``extra'' dimension, and for the unification scenario with 2 large extra dimensions, set an upper limit of 150 micrometers on the size of those dimensions.

  10. QM/MM Studies of the Triosephosphate Isomerase-Catalyzed Reaction

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Homesum_a_epg0_fpd_mmcf_m.xls" ,"Available from WebQuantityBonneville Power Administration wouldMass mapSpeedingProgramExemptionsProteinTotal natural gasPurchase,PyFEHM716,EnergyQM/MM

  11. TITLE: AUTHOR(S) SUBMITTED TO: Mm EVOLUTIO:l C: S!LICIC

    Office of Scientific and Technical Information (OSTI)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Homesum_a_epg0_fpd_mmcf_m.xls" ,"Available from WebQuantity of NaturalDukeWakefield MunicipalTechnicalInformation FederatedInformationTITLE: AUTHOR(S) SUBMITTED TO: Mm EVOLUTIO:l

  12. Optical-Infrared Properties of Faint 1.3 mm Sources Detected with ALMA

    E-Print Network [OSTI]

    Hatsukade, Bunyo; Yabe, Kiyoto; Seko, Akifumi; Makiya, Ryu; Akiyama, Masayuki

    2015-01-01

    We report optical-infrared (IR) properties of faint 1.3 mm sources (S_1.3mm = 0.2-1.0 mJy) detected with the Atacama Large Millimeter/submillimeter Array (ALMA) in the Subaru/XMM-Newton Deep Survey (SXDS) field. We searched for optical/IR counterparts of 8 ALMA-detected sources (>=4.0 sigma, the sum of the probability of spurious source contamination is ~1) in a K-band source catalog. Four ALMA sources have K-band counterpart candidates within a 0.4" radius. Comparison between ALMA-detected and undetected K-band sources in the same observing fields shows that ALMA-detected sources tend to be brighter, more massive, and more actively forming stars. While many of the ALMA-identified submillimeter-bright galaxies (SMGs) in previous studies lie above the sequence of star-forming galaxies in stellar mass--star-formation rate plane, our ALMA sources are located in the sequence, suggesting that the ALMA-detected faint sources are more like `normal' star-forming galaxies rather than `classical' SMGs. We found a regio...

  13. Design development for the 50mm Superconducting Super Collider dipole cryostat

    SciTech Connect (OSTI)

    Nicol, T.H.

    1991-03-01

    The cryostat of a Superconducting Super Collider (SSC) dipole magnet consists of all magnet components except the magnet assembly itself. It serves to support the magnet accurately and reliably within the vacuum vessel, provide all required cryogenic piping, and to insulate the cold mass from heat radiated and conducted from the environment. It must function reliably during storage, shipping and handling, normal magnet operation, quenches, and seismic excitations, and must be manufacturable at low cost. The major components of the cryostat are the vacuum vessel, thermal shields, multilayer insulation system, cryogenic piping, interconnections, and suspension system. The overall design of a cryostat for superconducting accelerator magnets requires consideration of fluid flow, proper selection of materials for their thermal and structural performance at both ambient and operating temperature, and knowledge of the environment to which the magnets will be subjected over the course their expected operating life. This paper describes the design of the current 50mm SSC collider dipole cryostat and includes discussions on the structural and thermal considerations involved in the development of each of the major systems. Where appropriate, comparisons will be made with the 40mm cryostat. 7 refs., 5 figs., 4 tabs.

  14. Design and Analysis of TQS01, a 90 mm Nb3Sn Model Quadrupole for LHC Luminosity Upgrade Based on a Key and Bladder Assembly

    E-Print Network [OSTI]

    Caspi, S.

    2008-01-01

    and Analysis of TQS01, a 90 mm Nb 3 Sn Model Quadrupole forStructure for an LHC 90 mm Nb 3 Sn quadrupole magnet”, IEEEal. , “Development of a 90-mm Nb3Sn Technological Quadrupole

  15. DEVELOPMENT OF A 40 mm BORE MAGNET CROSS SECTION WITH HIGH FIELD UNIFORMITY FOR THE 6.6T SSC DIPOLE

    E-Print Network [OSTI]

    Caspi, S.

    2010-01-01

    76SF00098. DEVELOPHENT OF A 40 mm BORE KAGNET CROSS SECTIONuniform dipole field. A 40 mm bo~e diameter winding cross3, 1986 DEVELOPMENT OF A 40 mm BORE MAGNET CROSS SECTION

  16. Imaging structure and composition homogeneity of 300 mm SiGe virtual substrates for advanced CMOS applications by scanning X-ray diffraction microscopy

    E-Print Network [OSTI]

    2015-01-01

    of New Materials on 300 mm Silicon Wafers. ECS Trans. 2012,Composition Homogeneity of 300 mm SiGe Virtual Substratesrelaxed bu?er layers on 300 mm Si(001) wafers treated with

  17. 5000 groove/mm multilayer-coated blazed grating with 33percent efficiency in the 3rd order in the EUV wavelength range

    E-Print Network [OSTI]

    Voronov, Dmitriy L.

    2010-01-01

    5000 groove/mm multilayer-coated blazed grating with 33%groove density 2400 grooves/mm optimized for diffraction inorder. 6 A denser 3000 grooves/mm grating has demonstrated

  18. First Lasing of Volume FEL (VFEL) at Wavelength Range $?\\sim $ 4-6 mm

    E-Print Network [OSTI]

    V. Baryshevsky; K. Batrakov; A. Gurinovich; I. Ilienko; A. Lobko; V. Moroz; P. Sofronov; V. Stolyarsky

    2001-07-18

    First lasing of volume free electron laser (VFEL) is described. The generating system consists of two metal diffraction grating with different spatial periods. The first grating creates the conditions for Smith Purcell emission mechanism. The second grating provides the distributed feedback for emitted wave. The length of diffraction grating is 10 cm. Electron beam pulse with a time duration $\\tau \\sim$ 10 ms has a sinusoidal form with the amplitude varied from 1 to ~10 kV. The measured microwave power reached the value of about 3-4 W in mm wavelength range. The generation stops at threshold current value. When the current tends to the threshold value, the region of generation tends to a narrow band near to 5 kV. At higher current values the radiation appears in electron energy range 5 - 7.5 KeV.

  19. A 1 mm Scintillating Fibre Tracker Readout by a Multi-anode Photomultiplier

    E-Print Network [OSTI]

    B. D. Leverington; M. Anelli; P. Campana; R. Rosellini

    2011-07-05

    This note describes a prototype particle tracking detector constructed with 1 mm plastic scintillating fibres with a 64 channel Hamamatsu H8500 flat-panel multi-anode photomultiplier readout. Cosmic ray tracks from an array of 11 gas-filled drift tubes were matched to signals in the scintillating fibres in order to measure the resolution and efficiency of tracks reconstructed in the fibre-based tracker. A GEANT4 detector simulation was also developed to compare cosmic ray data with MC results and is discussed in the note. Using the parameters measured in this experimental setup, modified fibre tracker designs are suggested to improve resolution and efficiency in future prototypes to meet modern detector specifications.

  20. The 1.3 mm Full-Stokes Polarization System at CARMA

    E-Print Network [OSTI]

    Hull, Charles L H

    2015-01-01

    The CARMA 1.3 mm polarization system consists of dual-polarization receivers that are sensitive to right- (R) and left-circular (L) polarization, and a spectral-line correlator that measures all four cross polarizations (RR, LL, LR, RL) on each of the 105 baselines connecting the 15 telescopes. Each receiver comprises a single feed horn, a waveguide circular polarizer, an orthomode transducer (OMT), two heterodyne mixers, and two low-noise amplifiers (LNAs), all mounted in a cryogenically cooled dewar. Here we review the basics of polarization observations, describe the construction and performance of key receiver components (circular polarizer, OMT, and mixers -- but not the correlator), and discuss in detail the calibration of the system, particularly the calibration of the R-L phase offsets and the polarization leakage corrections. The absolute accuracy of polarization position angle measurements was checked by mapping the radial polarization pattern across the disk of Mars. Transferring the Mars calibrati...

  1. A photocathode rf gun design for a mm-wave linac-based FEL

    SciTech Connect (OSTI)

    Nassiri, A.; Berenc, T,; Foster, J.; Waldschmidt, G.; Zhou, J.

    1995-07-01

    In recent years, advances in the rf gun technology have made it possible to produce small beam emittances suitable for short period microundulators which take advantage of the low emittance beam to reduce the wavelength of FELs. At the Advanced Photon Source, we are studying the design of a compact 50-MeV superconducting mm-wave linac-based FEL for the production of short wavelengths ({approximately}300 nm) to carry out FEL demonstration experiments. The electron source considered for the linac is a 30- GHz, 3 1/2-cell {pi}-mode photocathode rf gun. For cold model rf measurements a 15-GHz prototype structure was fabricated. Here we report on the design, numerical modelling and the initial cold-model rf measurement results on the 15-GHz prototype structure.

  2. Measurement of the large-scale anisotropy of the cosmic background radiation at 3mm

    SciTech Connect (OSTI)

    Epstein, G.L.

    1983-12-01

    A balloon-borne differential radiometer has measured the large-scale anisotropy of the cosmic background radiation (CBR) with high sensitivity. The antenna temperature dipole anistropy at 90 GHz (3 mm wavelength) is 2.82 +- 0.19 mK, corresponding to a thermodynamic anistropy of 3.48 +- mK for a 2.7 K blackbody CBR. The dipole direction, 11.3 +- 0.1 hours right ascension and -5.7/sup 0/ +- 1.8/sup 0/ declination, agrees well with measurements at other frequencies. Calibration error dominates magnitude uncertainty, with statistical errors on dipole terms being under 0.1 mK. No significant quadrupole power is found, placing a 90% confidence-level upper limit of 0.27 mK on the RMS thermodynamic quadrupolar anistropy. 22 figures, 17 tables.

  3. Hydrides of CeNi/sub 5/, MmNi/sub 5/, Ca/sub 0/ /sub 2/(Ce/sub 0/ /sub 65/Mm/sub 0/ /sub 35/)/sub 0/ /sub 8/Ni/sub 5/, Ca/sub 0/ /sub 2/Ce/sub 0/ /sub 8/Ni/sub 5/, Ca/sub 0/ /sub 2/Mm/sub 0/ /sub 8/Ni/sub 5/, and mixed CeNi/sub 5//MmNi/sub 5/

    SciTech Connect (OSTI)

    Lakner, J.F.; Chow, T.S.

    1982-09-01

    Six intermetallic alloys (CeNi/sub 5/, MmNi/sub 5/, Ca/sub 0/ /sub 2/(Ce/sub 0/ /sub 65/Mm/sub 0/ /sub 35/)/sub 0/ /sub 8/Ni/sub 5/, Ca/sub 0/ /sub 2/Ce/sub 0/ /sub 8/Ni/sub 5/, Ca/sub 0/ /sub 2/Mm/sub 0/ /sub 8/Ni/sub 5/, and a mixed alloy, CeNi/sub 5//MmNi/sub 5/) were investigated with respect to their suitability to provide high hydrogen capacity and their potential for use in providing substantial hydrogen pressure at both low and high temperatures. A second phase of our investigation dealt with ball-milling and hydriding and dehydriding cycles to produce fine particles for use in hydride powder transfer studies. A summary of several Van't Hoff plots is also included for hydride-forming alloys.

  4. The Growth of Black Holes and Their Host Spheroids in (Sub)mm-loud QSOs at High Redshift

    E-Print Network [OSTI]

    C. N. Hao; X. Y. Xia; S. Mao; Z. G. Deng; Hong Wu

    2007-04-24

    We study the growth of black holes and stellar population in spheroids at high redshift using several (sub)mm-loud QSO samples. Applying the same criteria established in an earlier work, we find that, similar to IR QSOs at low redshift, the far-infrared emission of these (sub)mm-loud QSOs mainly originates from dust heated by starbursts. By combining low-z IR QSOs and high-z (sub)mm-loud QSOs, we find a trend that the star formation rate ($\\Mstardot$) increases with the accretion rate ($\\Mdot$). We compare the values of $\\Mstardot/\\Mdot$ for submm emitting galaxies (SMGs), far-infrared ultraluminous/hyperluminous QSOs and typical QSOs, and construct a likely evolution scenario for these objects. The (sub)mm-loud QSO transition phase has both high $\\Mdot$ and $\\Mstardot$ and hence is important for establishing the correlation between the masses of black holes and spheroids.

  5. Freezing / Thawing mammalian cells (AG/2-96) 1. Grow cells to confluency in 100 mm plates.

    E-Print Network [OSTI]

    Ghosh, Anirvan

    Freezing / Thawing mammalian cells (AG/2-96) Freezing: 1. Grow cells to confluency in 100 mm plates ml per vial), seal, place between styrofoam tube holders, and freeze at -70 C. 7. Transfer tubes

  6. Sensitivity analysis of the MM5 weather model using automatic differentiation

    SciTech Connect (OSTI)

    Bischof, C.H. [Mathematics and Computer Science Division, Argonne National Laboratory, Argonne, Illinois 60439 (United States)] [Mathematics and Computer Science Division, Argonne National Laboratory, Argonne, Illinois 60439 (United States); Pusch, G.D. [Physics Department, Michigan State University, East Lansing, Michigan 48842 (United States)] [Physics Department, Michigan State University, East Lansing, Michigan 48842 (United States); Knoesel, R. [Mathematics and Computer Science Division, Argonne National Laboratory, Argonne, Illinois 60439 (United States)] [Mathematics and Computer Science Division, Argonne National Laboratory, Argonne, Illinois 60439 (United States)

    1996-11-01

    We present a general method for using automatic differentiation to facilitate model sensitivity analysis. Automatic differentiation techniques augment, in a completely mechanical fashion, an existing code such that it also simultaneously and efficiently computes derivatives. Our method allows the sensitivities of the code{close_quote}s outputs to its parameters and inputs to be determined with minimal human effort by exploiting the relationship between differentiation and formal perturbation theory. Employing this methodology, we performed a sensitivity study of the MM5 code, a mesoscale weather model jointly developed by Penn State University and the National Center for Atmospheric Research, that is composed of roughly 40,000 lines of Fortran 77 code. Our results show that automatic differentiation-computed sensitivities exhibit superior accuracy compared to divided difference approximations computed from finite-amplitude perturbations. We also comment on a numerically induced precursor wave that would almost certainly have been undetectable if one used a divided difference method. {copyright} {ital 1996 American Institute of Physics.}

  7. 1400 OPTICS LETTERS / Vol. 27, No. 16 / August 15, 2002 Low-loss, wide-angle Y splitter at 1.6-mm wavelengths built

    E-Print Network [OSTI]

    1400 OPTICS LETTERS / Vol. 27, No. 16 / August 15, 2002 Low-loss, wide-angle Y splitter at 1.6-mm at l 1.6 mm. Our device has a large splitting angle of 120± and a miniature size of 3 mm 3 3 mm of guiding and bending efficiency at l 1.5 1.6 mm wavelengths has also been carried out.3

  8. 3.2 mm lightcurve observations of (4) Vesta and (9) Metis with the Australia Telescope Compact Array

    E-Print Network [OSTI]

    T. G. Müller; P. J. Barnes

    2007-03-09

    (4) Vesta and (9) Metis are large main-belt asteroids with high albedos. With millimetre-observations at 93.0 and 95.5 GHz we characterised the emission properties of the surface material. The coverage of the full rotation period allowed a detailed study of the heterogeneity of the surface. The rotationally averaged fluxes are explained very well by our thermophysical model techniques when using an emissivity in the mm-range of about 0.6 for (4) Vesta and about 0.7 for (9) Metis. The mm-lightcurves follow for a large fraction of the rotation period the shape-introduced variations. The rotational phases with clear deviations are connected to structures which are visible in the HST images of (4) Vesta and the Keck AO-images of (9) Metis. The observed lightcurve amplitudes are peak-to-peak ~30% for (4) Vesta and ~25% for (9) Metis, while the shape-related amplitudes are only 5 and 4%, respectively. The emissivities at mm-wavelengths are lower than in the far-IR, confirming that particles with sizes of about 100 mikron influence the mm-behaviour. The 3-mm observations are very powerful for the study of asteroid surface heterogeneities.

  9. THE RAFFLESBULLETIN OF ZOOLOGY199644(1) Fig. 1. a, Orcovita saltatrix Ng & Tomascik, 1994,paratypemale (17.0by 13.0 mm) (MNHNB-

    E-Print Network [OSTI]

    Iliffe, Thomas M.

    ,paratypemale (17.0by 13.0 mm) (MNHNB- 22891); b, O. gracilipes, new species,holotype male (18.5 by 13.1 mm) (MNHN B-22892); c, O. mollitia, newspecies,holotypemale (12.6by 9.6 mm) (MNHN B-22895). #12;Ng et al. 2. a, Orcovitafictilia, newspecies,holotypemale (21.5by 15.3 mm)(NMCR); b, O. angulata

  10. .225 2 QQw 85 255mm 5:5 95 £< H an 882? .525 05 B @220 g 8 Ga ...

    E-Print Network [OSTI]

    on E “mm. :oaw: . 83:8 ta: 2? #53 @025 @822 g a 6 é 3: Gd 68 EN. 6 JV Am “8 2w Siam @228 .560 2t 35 850% on SS m .o n <6w was ESQ Route @ 2 8 “8 35 ...

  11. MALARIA I N NIGERIA: CDNSTRAINED CaYTINUXIS-TIE MARKDV MmLS A3R DISCRETE-TIME

    E-Print Network [OSTI]

    Cohen, Joel E.

    MALARIA I N NIGERIA: CDNSTRAINED CaYTINUXIS-TIE MARKDV MmLS A3R DISCRETE-TIME ~ I T U D I N t of northern Nigeria included 8 baseline surveys a t approximately - AHS(1OS) subject classifications (1970 grant SOC76-17706 t o Columbia University. #12;JOEL E. COHEN AND BURTON SINGER UALARIA I N NIGERIA 10

  12. e x ecu tiv e su mm a ry of accomp lishmen t s resea rch & development

    E-Print Network [OSTI]

    Subramanian, Venkat

    . Biswas) » Clean CoalTechnology Fund = $479,651 (R. Axelbaum) » Two NSF CAREER Awards: $400,000 (Y.-S. Jun is the first university to join the Advanced Coal Technology Consortia of the U.S.-China Clean Energy Researche x ecu tiv e su mm a ry of accomp lishmen t s resea rch & development » The Consortium for Clean

  13. Phase Referencing at the Palomar Testbed Interferometer B.F. Lane & M.M. Colavita (for the PTI Collaboration)

    E-Print Network [OSTI]

    Phase Referencing at the Palomar Testbed Interferometer B.F. Lane & M.M. Colavita (for the PTI Collaboration) Abstract We discuss implementation and testing of phase-referencing at the Palomar Testbed. The Instrument The Palomar Testbed Interferometer (PTI) is a long-baseline infrared interferometer installed

  14. A Virtual DSP System for Design Instruction of Power Converters AA.. KKeeyyhhaannii aanndd MM.. NN.. MMaarrwwaallii GGeerraalldd BBaauummggaarrttnneerr

    E-Print Network [OSTI]

    Baumgartner, Gerald

    1 A Virtual DSP System for Design Instruction of Power Converters AA.. KKeeyyhhaannii aanndd MM the development of an object oriented DSP based for design and control of power converters. The testbed `hard' switching power converters, a resonant converter utilizes a controlled series or parallel LC

  15. MM000422.R1 1 Abstract--In this paper we present a secure and robust content

    E-Print Network [OSTI]

    Chang, Shih-Fu

    MM000422.R1 1 Abstract--In this paper we present a secure and robust content based digital protecting the integrity of content and non-repudiation from the image sender. Content integrity protection means that the content isn't allowed to be modified in such a way that the content meaning is altered

  16. 0 10 20 30 40 50 60 70 80 90 100 Half spreading rate (mm per year)

    E-Print Network [OSTI]

    Müller, Dietmar

    60° 30° 0° 30° 60° 0 10 20 30 40 50 60 70 80 90 100 Half spreading rate (mm per year) Pacific Ocean you increase the speed of a continent ploughing through Earth's viscous, churning mantle? Kumar et al palaeomagnetic data and rates of seafloor spreading, and sets India apart from all its neighbours. Africa, Antarc

  17. WRF/MM5 User's Workshop, Boulder, CO, June 22-25, 2004, pp. 225-228. A Better Understanding of the Effects of

    E-Print Network [OSTI]

    Berleant, Daniel

    WRF/MM5 User's Workshop, Boulder, CO, June 22-25, 2004, pp. 225-228. A Better Understanding the impact of bugs in a well-known weather simulation system, MM5. The findings help fill a gap in knowledge questions. In the research reported here, bugs were artificially added to MM5. Their effects were analyzed

  18. BBIIOOLLOOGGYY SSEEMMIINNAARR AADD JJ UU NN CC TT AAPP PP OO II NN TT MM EE NN TT LLEE CC TT UU RR EE

    E-Print Network [OSTI]

    Brown, Sally

    BBIIOOLLOOGGYY SSEEMMIINNAARR AADD JJ UU NN CC TT AAPP PP OO II NN TT MM EE NN TT LLEE CC TT UU RR EE 44::0000 PPMM SSEE MM II NNAA RR PPHH YY SSII CCSS //AASS TTRR OONN OO MM YY AAUU DD .. AA110022

  19. Molecular Physics, Vol. 104, Nos. 57, 10 March10 April 2006, 701714 Geometry optimization with QM/MM methods II: Explicit

    E-Print Network [OSTI]

    Schlegel, H. Bernhard

    with QM/MM methods II: Explicit quadratic coupling T. VREVEN*y, M. J. FRISCHy, K. N. KUDINz, H. B QM/MM systems is usually carried out by alternating a second-order optimization of the QM region using internal coordinates (`macro-iterations'), and a first-order optimization of the MM region using

  20. Reflective Cracking Study: First-level Report on HVS Testing on Section 591RF - 45 mm MAC15TR-GOverlay

    E-Print Network [OSTI]

    Jones, David; Wu, R.; Harvey, John T

    2008-01-01

    Testing on Section 588RF — 90 mm AR4000-D Overlay (UCPRC-RR-Testing on Section 586RF — 45 mm MB15-G Overlay (UCPRC-RR-Testing on Section 591RF — 45 mm MAC15TR-G Overlay (UCPRC-

  1. Test Results of 15 T Nb3Sn Quadrupole Magnet HQ01 with a 120 mm Bore for the LHC Luminosity Upgrade

    E-Print Network [OSTI]

    Caspi, S.

    2012-01-01

    Magnet HQ01 with a 120 mm Bore for the L H C LuminosityFessia el ai, "Design of a 120 mm bore quadrupole for the LStructure for an L H C 90 mm N b S n quadrupole magnet,"

  2. Vol. 7, 1361-1368, October 1996 Cell Growth & Differentiation 1361 Action of Mm and Momi on Neoplasia in Ectopic Intestinal

    E-Print Network [OSTI]

    Dove, William

    Vol. 7, 1361-1368, October 1996 Cell Growth & Differentiation 1361 Action of Mm and Momi.] Abstract Mice heterozygous for Mm, a mutant allele of Apc, develop adenomas throughout the intestinal tract. Tumor multiplicity in Mm mice is influenced by genetic modifier loci. Previously, we mapped one

  3. BBIIOOLLOOGGYY SSEEMMIINNAARR AAFF FF II LL II AA TT EE AAPP PP OO II NN TT MM EE NN TT LLEE CC TT UU RR EE

    E-Print Network [OSTI]

    Brown, Sally

    BBIIOOLLOOGGYY SSEEMMIINNAARR AAFF FF II LL II AA TT EE AAPP PP OO II NN TT MM EE NN TT LLEE CC TT UU RR EE 44::0000 PPMM SSEE MM II NNAA RR PPHH YY SSII CCSS //AASS TTRR OONN OO MM YY AAUU DD .. AA

  4. Frequency synthesis using concurrency: Reaching a solution to a few classical and hard headed RF and mm-wave integrated circuit problems

    E-Print Network [OSTI]

    Jooyaie, Alborz

    2012-01-01

    18] A. H-T. Yu, et. al. , “a mm-wave arbitrary 2 N bandItoh, M.C.F. Chang, “A mm-wave arbitrary 2N band oscillatorand analysis of a 90 nm mm-wave oscillator using inductive

  5. A 19.1dBm Segmented Power-Mixer Based Multi-Gbps mm-Wave Transmitter in 32nm SOI CMOS

    E-Print Network [OSTI]

    Hajimiri, Ali

    A 19.1dBm Segmented Power-Mixer Based Multi-Gbps mm-Wave Transmitter in 32nm SOI CMOS Kaushik Abstract -- A high-power, fully-integrated, mm-wave power mixer based transmitter capable of generating case segmentation at 30% higher supply voltage. Index Terms -- mm-wave, , Power Mixer, CMOS Power

  6. The millimetre variability of M81* -- Multi-epoch dual frequency mm-observations of the nucleus of M81

    E-Print Network [OSTI]

    R. Schoedel; M. Krips; S. Markoff; R. Neri; A. Eckart

    2006-11-28

    There are still many open questions as to the physical mechanisms at work in Low Luminosity AGN that accrete in the extreme sub-Eddington regime. Simultaneous multi-wavelength studies have been very successful in constraining the properties of SgrA*, the extremely sub-Eddington black hole at the centre of our Milky Way. M81*, the nucleus of the nearby spiral galaxy M81, is an ideal source to extend the insights obtained on SgrA* toward higher luminosity AGN. Here we present observations at 3 and 1 mm that were obtained within the framework of a coordinated,multi-wavelength campaign on M81*. The continuum emission from M81* was observed during three epochs with the IRAM Plateau de Bure Interferometer simultaneously at wavelengths of 3 and 1 mm. We present the first flux measurements of M81* at wavelengths around 1 mm. We find that M81* is a continuously variable source with the higher variability observed at the shorter wavelength. Also, the variability at 3 and 1 mm appears to be correlated. Like SgrA*, M81* appears to display the strongest flux density and variability in the mm-to-submm regime. There remains still some ambiguity concerning the exact location of the turnover frequency from optically thick to optically thin emission. The observed variability time scales point to an upper size limit of the emitting region of the order 25 Schwarzschild radii. The data show that M81* is indeed a system with very similar physical properties to SgrA* and an ideal bridge toward high luminosity AGN. The data obtained clearly demonstrate the usefulness and, above all, the necessity of simultaneous multi-wavelength observations of LLAGN.

  7. Ability of the Confined Explosive Component Water Gap Test STANAG 4363 to Assess the Shock Sensitivity of MM-Scale Detonators

    SciTech Connect (OSTI)

    Lefrancois, A S; Roeske, F; Benterou, J; Tarver, C M; Lee, R S; Hannah, B

    2006-02-10

    The Explosive Component Water Gap Test (ECWGT) has been validated to assess the shock sensitivity of lead and booster components having a diameter larger than 5 mm. Several countries have investigated by experiments and numerical simulations the effect of confinement on the go/no go threshold for Pentaerythritol Tetranitrate (PETN) pellets having a height and diameter of 3 mm, confined by a steel annulus of wall thickness 1-3.5 mm. Confinement of the PETN by a steel annulus of the same height of the pellet with 1-mm wall thickness makes the component more sensitive (larger gap). As the wall thickness is increased to 2-mm, the gap increases a lesser amount, but when the wall thickness is increased to 3.5-mm a decrease in sensitivity is observed (smaller gap). This decrease of the water gap has been reproduced experimentally. Recent numerical simulations using Ignition and Growth model [1] for the PETN Pellet have reproduced the experimental results for the steel confinement up to 2 mm thick [2]. The presence of a stronger re-shock following the first input shock from the water and focusing on the axis have been identified in the pellet due to the steel confinement. The double shock configuration is well-known to lead in some cases to shock desensitization. This work presents the numerical simulations using Ignition and Growth model for LX16 (PETN based HE) and LX19 (CL20 based HE) Pellets [3] in order to assess the shock sensitivity of mm-scale detonators. The pellets are 0.6 mm in diameter and 3 mm length with different type of steel confinement 2.2 mm thick and 4.7 mm thick. The influence of an aluminum confinement is calculated for the standard LX 16 pellet 3 mm in diameter and 3 mm in height. The question of reducing the size of the donor charge is also investigated to small scale the test itself.

  8. A unique gun application for both high velocity and low velocity projectiles in a standard 155mm long tom gun

    SciTech Connect (OSTI)

    Garcia, J.R.

    1990-01-01

    The Terminal Ballistics Facility at Sandia National Laboratores in Albuquerque, New Mexico has developed an inexpensive and reliable capability for environmental testing of nuclear and kinetic energy weapon systems using the standard military 155 mm long tom gun. An unusual priming technique and charge configuration developed by Sandia National laboratories provides repeatable results such that payloads may be launched outside of the normal operating regime (both high and low) for the 155 mm gun. A 15 pound payload was reliably launched at 1000 fps with a breech pressure of 3000 psi. Another 20 pound payload was reliably launched to 5000 fps with a breech pressure of 50000 psi. A detailed description of charge configuration and test results is presented. 21 figs., 4 tabs.

  9. Accelerator Quality HTS Dipole Magnet Demonstrator Designs for the EuCARD-2, 5 Tesla 40 mm Clear Aperture Magnet

    E-Print Network [OSTI]

    Kirby, G A; Ballarino, A; Bottura, L; Chouika, N; Clement, S; Datskov, V; Fajardo, L; Fleiter, J; Gauthier, R; Gentini, L; Lambert, L; Lopes, M; Perez, J C; de Rijk, G; Rijllart, A; Rossi, L; ten Kate, H; Durante, M; Fazilleau, P; Lorin, C; Härö, E; Stenvall, A; Caspi, S; Marchevsky, M; Goldacker, W; Kario, A

    2015-01-01

    Future high-energy accelerators will need very high magnetic fields in the range of 20 T. The EuCARD-2 work-package-10 is a collaborative push to take HTS materials into an accelerator quality demonstrator magnet. The demonstrator will produce 5 T standalone and between 17 T and 20 T, when inserted into the 100 mm aperture of Fresca-2 high field out-sert magnet. The HTS magnet will demonstrate the field strength and field quality that can be achieved. An effective quench detection and protection system will have to be developed to operate with the HTS superconducting materials. This paper presents a ReBCO magnet design using multi strand Roebel cable that develops a stand-alone field of 5 T in a 40 mm clear aperture and discusses the challenges associated with good field quality using this type of material. A selection of magnet designs is presented as result of a first phase of development.

  10. Accelerator Quality HTS Dipole Magnet Demonstrator designs for the EuCARD-2, 5 Tesla 40 mm Clear Aperture Magnet

    E-Print Network [OSTI]

    Kirby, G; Ballarino, A; Bottura, L; Chouika, N; Clement, S; Datskov, V; Fajardo, L; Fleiter, J; Gauthier, R; Lambert, L; Lopes, M; Perez, J; DeRijk, G; Rijllart, A; Rossi, L; Ten Kate, H; Durante, M; Fazilleau, P; Lorin, C; Haro, E; Stenvall, A; Caspi, S; Marchevsky, M; Goldacker, W; Kario, A

    2014-01-01

    Future high-energy accelerators will need very high magnetic fields in the range of 20 T. The EuCARD-2 work-package-10 is a collaborative push to take HTS materials into an accelerator quality demonstrator magnet. The demonstrator will produce 5 T standalone and between 17 T and 20 T, when inserted into the 100 mm aperture of Fresca-2 high field out-sert magnet. The HTS magnet will demonstrate the field strength and field quality that can be achieved. An effective quench detection and protection system will have to be developed to operate with the HTS superconducting materials. This paper presents a ReBCO magnet design using multi strand Roebel cable that develops a stand-alone field of 5 T in a 40 mm clear aperture and discusses the challenges associated with good field quality using this type of material. A selection of magnet designs is presented as result of a first phase of development.

  11. How large should the QM region be in QM/MM calculations? The case of catechol O-methyltransferase

    E-Print Network [OSTI]

    Heather J. Kulik; Jianyu Zhang; Judith P. Klinman; Todd J. Martinez

    2015-05-21

    Hybrid quantum mechanical-molecular mechanical (QM/MM) simulations are widely used in studies of enzymatic catalysis. Up until now, it has usually been cost prohibitive to determine the convergence of these calculations with respect to the size of the QM region. Recent advances in reformulating electronic structure algorithms for stream processors such as graphical processing units have made QM/MM calculations of optimized reaction paths with QM regions comprising up to O(10^3) atoms feasible. Here, we leverage these GPU-accelerated quantum chemistry methods to investigate catalytic properties in catechol O-methyltransferase. Using QM regions ranging in size from the reactant only (63 atoms) up to nearly one-third of the entire protein (940 atoms), we show that convergence of properties such as the activation energy of the catalyzed reaction can be quite slow. Convergence to within chemical accuracy for this case requires a quantum mechanical region with approximately 500 atoms. These results call for a more careful determination of QM region sizes in future QM/MM studies of enzymes.

  12. Magnetic Materials (MM)

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Homesum_a_epg0_fpd_mmcf_m.xls" ,"Available from WebQuantityBonneville Power Administration would likeUniverseIMPACTThousandReport) |Administration Savannah River

  13. The Three-mm Ultimate Mopra Milky Way Survey. I. Survey Overview, Initial Data Releases, and First Results

    E-Print Network [OSTI]

    Barnes, Peter J; Indermuehle, Balthasar; O'Dougherty, Stefan N; Lowe, Vicki; Cunningham, Maria R; Hernandez, Audra K; Fuller, Gary A

    2015-01-01

    We describe a new mm-wave molecular-line mapping survey of the southern Galactic Plane and its first data releases. The Three-mm Ultimate Mopra Milky Way Survey (ThrUMMS) maps a 60{\\deg}x2{\\deg} sector of our Galaxy's fourth quadrant, using a combination of fast mapping techniques with the Mopra radio telescope, simultaneously in the J=1-0 lines of $^{12}$CO, $^{13}$CO, C$^{18}$O, and CN near 112 GHz at ~arcminute and ~0.3 km s$^{-1}$ resolution, with ~2 K channel$^{-1}$ sensitivity for $^{12}$CO and ~1 K channel$^{-1}$ for the other transitions. The calibrated data cubes from these observations are made available to the community after processing through our pipeline. Here, we describe the motivation for ThrUMMS, the development of new observing techniques for Mopra, and how these techniques were optimised to the objectives of the survey. We showcase some sample data products and describe the first science results on CO-isotopologue line ratios. These vary dramatically across the Galactic Plane, indicating a...

  14. How large should the QM region be in QM/MM calculations? The case of catechol O-methyltransferase

    E-Print Network [OSTI]

    Kulik, Heather J; Klinman, Judith P; Martinez, Todd J

    2015-01-01

    Hybrid quantum mechanical-molecular mechanical (QM/MM) simulations are widely used in studies of enzymatic catalysis. Up until now, it has usually been cost prohibitive to determine the convergence of these calculations with respect to the size of the QM region. Recent advances in reformulating electronic structure algorithms for stream processors such as graphical processing units have made QM/MM calculations of optimized reaction paths with QM regions comprising up to O(10^3) atoms feasible. Here, we leverage these GPU-accelerated quantum chemistry methods to investigate catalytic properties in catechol O-methyltransferase. Using QM regions ranging in size from the reactant only (63 atoms) up to nearly one-third of the entire protein (940 atoms), we show that convergence of properties such as the activation energy of the catalyzed reaction can be quite slow. Convergence to within chemical accuracy for this case requires a quantum mechanical region with approximately 500 atoms. These results call for a more ...

  15. Electron dynamics in complex environments with real-time time dependent density functional theory in a QM-MM framework

    SciTech Connect (OSTI)

    Morzan, Uriel N.; Ramírez, Francisco F.; Scherlis, Damián A. E-mail: mcgl@qb.ffyb.uba.ar; Lebrero, Mariano C. González E-mail: mcgl@qb.ffyb.uba.ar

    2014-04-28

    This article presents a time dependent density functional theory (TDDFT) implementation to propagate the Kohn-Sham equations in real time, including the effects of a molecular environment through a Quantum-Mechanics Molecular-Mechanics (QM-MM) hamiltonian. The code delivers an all-electron description employing Gaussian basis functions, and incorporates the Amber force-field in the QM-MM treatment. The most expensive parts of the computation, comprising the commutators between the hamiltonian and the density matrix—required to propagate the electron dynamics—, and the evaluation of the exchange-correlation energy, were migrated to the CUDA platform to run on graphics processing units, which remarkably accelerates the performance of the code. The method was validated by reproducing linear-response TDDFT results for the absorption spectra of several molecular species. Two different schemes were tested to propagate the quantum dynamics: (i) a leap-frog Verlet algorithm, and (ii) the Magnus expansion to first-order. These two approaches were confronted, to find that the Magnus scheme is more efficient by a factor of six in small molecules. Interestingly, the presence of iron was found to seriously limitate the length of the integration time step, due to the high frequencies associated with the core-electrons. This highlights the importance of pseudopotentials to alleviate the cost of the propagation of the inner states when heavy nuclei are present. Finally, the methodology was applied to investigate the shifts induced by the chemical environment on the most intense UV absorption bands of two model systems of general relevance: the formamide molecule in water solution, and the carboxy-heme group in Flavohemoglobin. In both cases, shifts of several nanometers are observed, consistently with the available experimental data.

  16. To obtain representative temperatures, sensors were made with a length of 35 cm. The stainless steel needles have a diameter of 3 mm. Inside are five

    E-Print Network [OSTI]

    Haak, Hein

    To obtain representative temperatures, sensors were made with a length of 35 cm. The stainless steel needles have a diameter of 3 mm. Inside are five Platinum Pt-100 sensors, that are cascaded

  17. Methanol Masers Observations in the 3-mm Bandwidth at the Radio Telescope RT-22 CrAO

    E-Print Network [OSTI]

    S. Yu. Zubrin; A. V. Antyufeyev; V. V. Myshenko; V. M. Shulga

    2007-12-10

    We report the beginning of the astronomical masers investigations in the 3-mm bandwidth at the radio telescope RT-22 (CrAO, Ukraine). For this purpose the special complex for maser lines investigation in 85...115 GHz frequency band is developed. It is made on the base of the low noise cryogenic Shottky-diode receiver and the high resolution Fourier-spectrometer. The cryogenic receiver has the DSB noise temperature less than 100K. The spectral channel separation of the Fourier-spectrometer is about 4kHz and the spectrometer bandwidth is 8 MHz. Results of maser observations of 8$^{0}-7^{1} $A$^{+}$ transition of methanol (95.169 GHz) towards DR-21(OH), DR-21W and NGC7538 are in good agreement with early obtained results by other authors. On the basis of the analysis of the location of masers in the NGC7538 direction we can assume that the origin of all known class I methanol masers in this region is connected with existing molecular outflows from young stars.

  18. A 0.042 mm^2 programmable biphasic stimulator for cochlear implants suitable for a large number of channels

    E-Print Network [OSTI]

    Ngamkham, W; Serdijn, W A; Bes, C J; Briaire, J J; Frijns, J H M

    2015-01-01

    This paper presents a compact programmable biphasic stimulator for cochlear implants. By employing double-loop negative feedback, the output impedance of the current generator is increased, while maximizing the voltage compliance of the output transistor. To make the stimulator circuit compact, the stimulation current is set by scaling a reference current using a two stage binary-weighted transistor DAC (comprising a 3 bit high-voltage transistor DAC and a 4 bit low-voltage transistor DAC). With this structure the power consumption and the area of the circuit can be minimized. The proposed circuit has been implemented in AMS 0.18um high-voltage CMOS IC technology, using an active chip area of about 0.042mm^2. Measurement results show that proper charge balance of the anodic and cathodic stimulation phases is achieved and a dc blocking capacitor can be omitted. The resulting reduction in the required area makes the proposed system suitable for a large number of channels.

  19. Mathematical Model for the Optimal Utilization Percentile in M/M/1 Systems: A Contribution about Knees in Performance Curves

    E-Print Network [OSTI]

    Gonzalez-Horta, Francisco A; Ramirez-Cortes, Juan M; Martinez-Carballido, Jorge; Buenfil-Alpuche, Eldamira

    2011-01-01

    Performance curves of queueing systems can be analyzed by separating them into three regions: the flat region, the knee region, and the exponential region. Practical considerations, usually locate the knee region between 70-90% of the theoretical maximum utilization. However, there is not a clear agreement about where the boundaries between regions are, and where exactly the utilization knee is located. An open debate about knees in performance curves was undertaken at least 20 years ago. This historical debate is mainly divided between those who claim that a knee in the curve is not a well defined term in mathematics, or it is a subjective and not really meaningful concept, and those who define knees mathematically and consider their relevance and application. In this paper, we present a mathematical model and analysis for identifying the three mentioned regions on performance curves for M/M/1 systems; specifically, we found the knees, or optimal utilization percentiles, at the vertices of the hyperbolas tha...

  20. Operating characteristics of a 7. 6 mm (0. 30 inch) diameter two-stage light-gas gun

    SciTech Connect (OSTI)

    Susoeff, A R; Hawke, R S; Bowen, P R; Greenwood, D W; Marshall, F R

    1992-07-01

    a series of tests was conducted to determine the operating requirements needed to obtain maximum projectile velocity within the engineering design limits of a two-stage light-gas gun with a 7.6 mm (0.30 inch) diameter bore launch tube. The tests were conducted in a medium vacuum flight range. Previous experience with the gun was used to establish the minimum requirements for optimum efficiency. Two operating parameters, propellant load and drive gas pressure, were varied in order to find an initial optimum operating condition at a conservative propellant load. Propellant load and driver gas pressure were then incrementally increased. This procedure was methodically applied until significant mechanical deformation of a critical gun component took place. This report presents the results of these tests. Projectile velocity was measured to better than 3 percent accuracy using a magnetic induction technique. A 0.485 gram polycarbonate projectile was launched to a velocity of 7.77 km/s during the tests. 13 refs.

  1. The MagLab's ultra-wide-bore (105mm) 21.1T NMR/MRI magnet provides an opportunity to use low gamma, low

    E-Print Network [OSTI]

    McQuade, D. Tyler

    The MagLab's ultra-wide-bore (105mm) 21.1T NMR/MRI magnet provides an opportunity to use low gamma, low sensitive nuclei for MR imaging. The potential of nuclei such as chlorine remains largely and the capability of MRI at ultra high magnetic fields to observe glioma. The finding of an increased concentration

  2. 10 to 70% methanol in 50 mM KH2PO4 over 25 min, 10 ml/min, monitor at 380 nm). Next, the HPLC-

    E-Print Network [OSTI]

    Gao, Jinming

    10 to 70% methanol in 50 mM KH2PO4 over 25 min, 10 ml/min, monitor at 380 nm). Next, the HPLC- purified mixture was desalted on the same column (methanol was removed on a rotary evaporator, and the sample loaded in H2O and eluted with 90% methanol) and lyophilized, yielding the purified Nvoc

  3. Machine Design -2 Consider a machined 60mm diameter shaft made of AISI 1020 HR (Sut = 380 MPa at 20C) quenched

    E-Print Network [OSTI]

    Battaglia, Francine

    Machine Design - 2 Consider a machined 60mm diameter shaft made of AISI 1020 HR (Sut = 380 MPa at 20°C) quenched steel shown below. The shaft is supported by bearings at the ends. Mounted upon the shaft are two collars through which fluctuating loads are applied as shown. A groove is machined

  4. Palomar Testbed Interferometer -Update B.F. Lane a , M.M. Colavita b , A.F. Boden b , P.R. Lawson b (for the PTI Collaboration)

    E-Print Network [OSTI]

    Palomar Testbed Interferometer - Update B.F. Lane a , M.M. Colavita b , A.F. Boden b , P.R. Lawson, 4800 Oak Grove Dr., Pasadena, CA., 91109, USA. ABSTRACT The Palomar Testbed Interferometer (PTI) is a long-baseline near-infrared interferometer operating at Palomar Observatory, CA. The interferometer has

  5. AzTEC/ASTE 1.1-mm survey of SSA22: Counterpart identification and photometric redshift survey of submillimetre galaxies

    E-Print Network [OSTI]

    Umehata, H.; Tamura, Y.; Kohno, K.; Hatsukade, B.; Scott, K. S.; Kubo, M.; Yamada, T.; Ivison, R. J.; Cybulski, R.; Aretxaga, I.; Austermann, J.; Hughes, D. H.; Ezawa, H.; Hayashino, T.; Ikarashi, S.; Iono, D.; Kawabe, R.; Matsuda, Y.; Matsuo, H.; Nakanishi, K.; Oshima, T.; Perera, Thushara A.; Takata, T.; Wilson, Graham Wallace; Yun, M. S.

    2014-06-01

    We present the results from a 1.1-mm imaging survey of the SSA22 field, known for having an overdensity of z = 3.1 Lyman ? emitting galaxies (LAEs), taken with the astronomical thermal emission camera (AzTEC) on the Atacama ...

  6. A self-consistent MoD-WM/MM structural refinement method: characterization of hydrogen bonding in the orytricha nova G-1uar

    SciTech Connect (OSTI)

    Batista, Enrique R [Los Alamos National Laboratory; Newcomer, Micharel B [YALE UNIV; Raggin, Christina M [YALE UNIV; Gascon, Jose A [YALE UNIV; Loria, J Patrick [YALE UNIV; Batista, Victor S [YALE UNIV

    2008-01-01

    This paper generalizes the MoD-QM/MM hybrid method, developed for ab initio computations of protein electrostatic potentials [Gasc6n, l.A.; Leung, S.S.F.; Batista, E.R.; Batista, V.S. J. Chem. Theory Comput. 2006,2, 175-186], as a practical algorithm for structural refinement of extended systems. The computational protocol involves a space-domain decomposition scheme for the formal fragmentation of extended systems into smaller, partially overlapping, molecular domains and the iterative self-consistent energy minimization of the constituent domains by relaxation of their geometry and electronic structure. The method accounts for mutual polarization of the molecular domains, modeled as Quantum-Mechanical (QM) layers embedded in the otherwise classical Molecular-Mechanics (MM) environment according to QM/MM hybrid methods. The method is applied to the description of benchmark models systems that allow for direct comparisons with full QM calculations, and subsequently applied to the structural characterization of the DNA Oxytricha nova Guanine quadruplex (G4). The resulting MoD-QM/MM structural model of the DNA G4 is compared to recently reported highresolution X-ray diffraction and NMR models, and partially validated by direct comparisons between {sup 1}H NMR chemical shifts that are highly sensitive to hydrogen-bonding and stacking interactions and the corresponding theoretical values obtained at the density functional theory DFT QM/MM (BH&H/6-31 G*:Amber) level in conjunction with the gauge independent atomic orbital (GIAO) method for the ab initio self consistent-field (SCF) calculation of NMR chemical shifts.

  7. The effect of temperature and gas flow on the physical vapour growth of mm-scale rubrene crystals for organic FETs

    E-Print Network [OSTI]

    A. R. Ullah; A. P. Micolich; J. W. Cochrane; A. R. Hamilton

    2007-11-12

    There has recently been significant interest in rubrene single-crystals grown using physical vapour transport techniques due to their application in high-mobility organic field-effect transistor (OFET) devices. Despite numerous studies of the electrical properties of such crystals, there has only been one study to date focussing on characterising and optimising the crystal growth as a function of the relevant growth parameters. Here we present a study of the dependence of the yield of useful crystals (defined as crystals with at least one dimension of order 1 mm) on the temperature and volume flow of carrier gas used in the physical vapour growth process.

  8. Coupling MM5 with ISOLSM:

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Homesum_a_epg0_fpd_mmcf_m.xls" ,"Available from WebQuantityBonneville Power Administration would like submit the followingConcentratingPortalCoolCoronaryCosts Associated4-Year/%2A Yun

  9. Photometric study of southern SU UMa-type dwarf novae and candidates -- III: NSV 10934, MM Sco, AB Nor, CAL 86

    E-Print Network [OSTI]

    T. Kato; P. Nelson; C. Stockdale; B. Monard; T. Richards; R. Stubbings; H. Yamaoka; B. Heathcote; R. Santallo

    2003-10-01

    We photometrically observed four southern dwarf novae in outburst (NSV 10934, MM Sco, AB Nor and CAL 86). NSV 10934 was confirmed to be an SU UMa-type dwarf nova with a mean superhump period of 0.07478(1) d. This star also showed transient appearance of quasi-periodic oscillations (QPOs) during the final growing stage of the superhumps. Combined with the recent theoretical interpretation and with the rather unusual rapid terminal fading of normal outbursts, NSV 10934 may be a candidate intermediate polar showing SU UMa-type properties. The mean superhump periods of MM Sco and AB Nor were determined to be 0.06136(4) d and 0.08438(2) d, respectively. We suggest that AB Nor belongs to a rather rare class of long-period SU UMa-type dwarf novae with low mass-transfer rates. We also observed an outburst of the suspected SU UMa-type dwarf nova CAL 86. We identified this outburst as a normal outburst and determined the mean decline rate of 1.1 mag/d.

  10. 2/1/2014 Micro Windmill-Powered Chargers -This 1.88MM Wide Windmill Can Recharge Your Smartphone Battery(VIDEO) http://www.trendhunter.com/trends/windmill-powered 1/7

    E-Print Network [OSTI]

    Chiao, Jung-Chih

    2/1/2014 Micro Windmill-Powered Chargers - This 1.88MM Wide Windmill Can Recharge Your Smartphone Battery(VIDEO) http://www.trendhunter.com/trends/windmill-powered 1/7 Select Category TECH Wholesale Solar: Jan 22, 2014 · References: youtube and gizmag This 1.88MM Wide Windmill Can Recharge Your Smartphone

  11. Comparing Terminal Performance of .357 SIG and 9mm Bullets in Ballistic Gelatin Using Retarding Force Analysis from High Speed Video

    E-Print Network [OSTI]

    Keys, Elizabeth; Courtney, Michael

    2015-01-01

    High-speed video has emerged as an valuable tool for quantifying bullet performance in ballistic gelatin. This paper presents the results of testing four .357 SIG bullets using high-speed video of bullet impacts in ballistic gelatin to determine retarding force curves, permanent cavities, temporary cavities, and energy deposit vs. penetration depth. Since the methods are identical, results are meaningfully compared with four 9mm NATO bullets studied in an earlier project. Though .357 SIG bullets perform slightly better due to higher impact energy, the principal finding is that there is a much bigger difference in performance between the best and worst performing bullets in each cartridge than there is between bullets of similar design in the two cartridges. In each cartridge, higher performing expanding bullets (jacketed hollow points) outperform non-expanding bullets (full metal jacket) by a wide margin, showing a much higher probability of rapid incapacitation according to an Army Research Laboratory model ...

  12. An AzTEC 1.1-mm Survey for ULIRGs in the field of the Galaxy Cluster MS 0451.6-0305

    E-Print Network [OSTI]

    Wardlow, J L; Wilson, G W; Yun, M S; Coppin, K E K; Cybulski, R; Geach, J E; Ivison, R J; Aretxaga, I; Austermann, J E; Edge, A C; Fazio, G G; Huang, J; Hughes, D H; Kodama, T; Kang, Y; Kim, S; Mauskopf, P D; Perera, T A; Scott, K S

    2009-01-01

    We have undertaken a deep (sigma~1.1 mJy) 1.1-mm survey of the z=0.54 cluster MS 0451.6-0305 using the AzTEC camera on the James Clerk Maxwell Telescope. We detect 36 sources with S/N>3.5 in the central 0.10 deg^2 and present the AzTEC map, catalogue and number counts. We identify counterparts to 18 sources (50%) using radio, mid-infrared, Spitzer IRAC and Submillimeter Array data. Optical, near- and mid-infrared spectral energy distributions are compiled for the 14 of these galaxies with detectable counterparts, which are expected to contain all likely cluster members. We then use photometric redshifts and colour selection to separate background galaxies from potential cluster members and test the reliability of this technique using archival observations of submillimetre galaxies. We find two potential MS 0451-03 members, which, if they are both cluster galaxies have a total star-formation rate (SFR) of ~100 solar masses per year -- a significant fraction of the combined SFR of all the other galaxies in MS 0...

  13. A mm-Scale Dosimetry System Based on Optically Stimulated Luminescence of Beryllium Oxide for Investigation of Dose Rate Profiles in Constricted Environments - 12219

    SciTech Connect (OSTI)

    Sommer, Marian; Jahn, Axel; Sommer, Dora; Henniger, Juergen [Technische Universitaet Dresden, Institute for Nuclear and Particle Physics, Radiation Physics Group, D-01062 Dresden (Germany); Praetorius, Reiner M. [Wiederaufarbeitungsanlage Karlsruhe Rueckbau- und Entsorgungs- GmbH, POB 1263, D-76339 Eggenstein-Leopoldshafen (Germany)

    2012-07-01

    The dismantling of the former German fuel reprocessing research center Wiederaufbeitungsanlage Karlsruhe requires extensive investigations of contamination and dose rate inside of the shielded areas. Particularly for first the exploration of radiation field existing thermo-element pipes may offer access to the tanks and to other interesting points without the risk of contamination. Because of their small dimension, almost no active dosimetry systems are able to measure inside the pipes. New mm-scale luminescence dosimeters in combination with a packing and transport technique are presented. The dosimeters could measure doses from 0.1 mGy up to more than 100 Gy. Hence, over the possible exposure time durations, dose rates from ?Gyh{sup -1} up to 1000 Gyh{sup -1} are ascertainable. For potential users the system opens the opportunity for investigation of dose rates inside of shielding and in contaminated environments. Particularly in constricted environments the technique is a unique solution for dose and dose rate measurement tasks. Within the linear dose range up to several ten Gy, the uncertainty of the results is less than 5%. 100 Gy-doses can be specified within 20%, with individual high dose calibration of the detectors even better. For WAK and other potential users the system offers the opportunity to investigate dose rates inside of shieldings and in contaminated environments. Particularly in constricted environments the technique is an unique solution for dose and dose rate measurements. (authors)

  14. High moisture corn stover pelleting in a flat die pellet mill fitted with a 6 mm die: physical properties and specific energy consumption

    DOE Public Access Gateway for Energy & Science Beta (PAGES Beta)

    Tumuluru, Jaya Shankar

    2015-06-15

    The quality and specific energy consumption (SEC) of the biomass pellets produced depend upon pelleting process conditions. The present study includes understanding the effect of feedstock moisture in the range of 28–38% (wet basis [w.b.]) and preheating in the range of 30–110°C at two die speeds of 40 and 60 Hz on the physical properties and SEC. A flat die pellet mill fitted with a 6 mm die was used in the present study. The physical properties of pellets such as moisture content, unit, bulk and tapped density, durability, and expansion ratio and SEC of the pelleting process are measured.more »The results indicate that the pellets produced have durability values in the range of 87–98%, and unit bulk and tapped density in the range of 670–1100, 375–575, and 420–620 kg/m³. Increasing the feedstock moisture content from 33% to 38% (w.b) decreased the unit, bulk and tapped density by about 30–40%. Increasing feedstock moisture content increased the expansion ratio and decreased the density values. A higher feedstock moisture content of 38% (w.b.) and higher preheating temperature of 110°C resulted in lower density and a higher expansion ratio, which can be attributed to flash off of moisture as the material extrudes out of the die. The SEC was in the range of 75–275 kWh/ton. Higher feedstock moisture content of 38% (w.b.) and a lower die speed of 40 Hz increased the SEC, whereas lower to medium preheating temperature (30–70°C), medium feedstock moisture content of 33% (w.b.), and a higher die speed of 60 Hz minimized the SEC to « less

  15. Computation of the free energy due to electron density fluctuation of a solute in solution: A QM/MM method with perturbation approach combined with a theory of solutions

    SciTech Connect (OSTI)

    Suzuoka, Daiki; Takahashi, Hideaki Morita, Akihiro

    2014-04-07

    We developed a perturbation approach to compute solvation free energy ?? within the framework of QM (quantum mechanical)/MM (molecular mechanical) method combined with a theory of energy representation (QM/MM-ER). The energy shift ? of the whole system due to the electronic polarization of the solute is evaluated using the second-order perturbation theory (PT2), where the electric field formed by surrounding solvent molecules is treated as the perturbation to the electronic Hamiltonian of the isolated solute. The point of our approach is that the energy shift ?, thus obtained, is to be adopted for a novel energy coordinate of the distribution functions which serve as fundamental variables in the free energy functional developed in our previous work. The most time-consuming part in the QM/MM-ER simulation can be, thus, avoided without serious loss of accuracy. For our benchmark set of molecules, it is demonstrated that the PT2 approach coupled with QM/MM-ER gives hydration free energies in excellent agreements with those given by the conventional method utilizing the Kohn-Sham SCF procedure except for a few molecules in the benchmark set. A variant of the approach is also proposed to deal with such difficulties associated with the problematic systems. The present approach is also advantageous to parallel implementations. We examined the parallel efficiency of our PT2 code on multi-core processors and found that the speedup increases almost linearly with respect to the number of cores. Thus, it was demonstrated that QM/MM-ER coupled with PT2 deserves practical applications to systems of interest.

  16. MHD Simulations of a Supernova-driven ISM Alex S Hill1, MR Joung2,5, RA Benjamin3, LM Haffner1, C Klingenberg4, M-M Mac Low5, K Waagan6, KA Wood7

    E-Print Network [OSTI]

    Wisconsin at Madison, University of

    Klingenberg4, M-M Mac Low5, K Waagan6, KA Wood7 1U of Wisconsin-Madison, 2Columbia U, 3U of Wisconsin, implying that the simulations have more low density and more high density gas than the real ISM (Wood et al, resulting in the near-absence of the warm ionized medium at those heights (Wood et al 2010). 3) The model

  17. Acid Washed Glass Beads 1. Weigh 50 g of 0.5 mm glass beads (Sigma G-9268, 425-600 m) into a 100 ml-orange cap Pyrex

    E-Print Network [OSTI]

    Aris, John P.

    Acid Washed Glass Beads 1. Weigh 50 g of 0.5 mm glass beads (Sigma G-9268, 425-600 µm) into a 100 ml-orange cap Pyrex bottle. The volume of glass beads should be no more than 1/5 of the volume of the bottle used for washes. To scale up, use 100 g of glass beads and a 250 ml orange cap Pyrex bottle. 2

  18. RNA Extraction and Labeling 1. To IP pellet (~ 25 l vol), add 175 l of: 10 mM HEPES-NaOH, pH 7.5

    E-Print Network [OSTI]

    Aris, John P.

    85 RNA Extraction and Labeling 1. To IP pellet (~ 25 µl vol), add 175 µl of: 10 mM HEPES-NaOH, pH 7 Speed-Vac. 7. Labeling 3' ends. To each pellet, add 10 µl containing: 1 X NEB RNA Ligase buffer 10% DMSO precipitate. Use DEPC-treated 3M NaOAc, pH 5. Wash with 75% EtOH and dry. 12. Resuspend pellet completely in 5

  19. A conventional one-channel Thomson scattering (TS) system was implemented to measure the electron temperature and density profiles on the ETE tokamak plasma with a resolution of 15 mm along 50 cm inside the plasma. The TS is based on a 10 J Q-switched rub

    E-Print Network [OSTI]

    temperature and density profiles on the ETE tokamak plasma with a resolution of 15 mm along 50 cm inside.5mmx1.5mm that is spectral analyzed by a 5-channel filter polychromator. Temperatures from 20 eV to 160 uses large core monofibers (d = 0.8 mm, NA = 0.39, average attenuation: 7 dB/Km) with micro-lenses (d

  20. Physical Consequences of a Momenta-Transfering Particle Theory of Induced Gravity and New Measurements Indicating Variation from Inverse Square Law at Length Scale of .1 mm: Statistical Time Properties of Gravitational Interaction and Analysis Thereof

    E-Print Network [OSTI]

    Gary Christopher Vezzoli

    2001-04-04

    This work presents physical consequences of our theory of induced gravity (Ref.1) regarding: 1) the requirement to consider shape and materials properties when calculating graviton cross section collision area; 2) use of Special Relativity; 3) implications regarding the shape of cosmos; 4) comparison to explanations using General Relativity; 5) properties of black holes; 6) relationship to the strong force and the theorized Higgs boson; 7) the possible origin of magnetic attraction; 8) new measurements showing variation from gravitational inverse square behavior at length scales of 0.1 mm and relationship to the Cosmological constant, and proof of the statistical time properties of the gravitational interaction.

  1. Le JJ/MM/AAAA RELATIONS INTERNATIONALES

    E-Print Network [OSTI]

    Sart, Remi

    and industrial base of 60 000 companies with some big names : Michelin, Limagrain, Volvic IBM... sectors of Engineering University Institute of Computer Science and Modelling 1 University Institute of Technology (2;Research 25 laboratories centred on 6 main areas of research: - Mathematics and computer sciences - Science

  2. Concept : Cell Yield Glucose, mM

    E-Print Network [OSTI]

    Málaga, Universidad de

    on Limiting Substrate. Specific growth rate reaches a maximum value of 0.5 h-1. Value of KS here is 0.5 g L-1 body, degeneration) Limitation in the length of cDNA Lacks post-translational modification específico (Baculovirus) Cultivo fastidioso Tiempo de crecimiento my lento (tiempo de doblaje es 20h) #12

  3. mm-Wave Phase Shifters and Switches

    E-Print Network [OSTI]

    Adabi Firouzjaei, Ehsan

    2010-01-01

    a transformer-based shunt switch and its equivalent circuitTraditional shunt switches occupy a large footprint as a2.4 Transformer based switch design example in 90nm CMOS

  4. Totsl length (mm) Sample 95% confidence

    E-Print Network [OSTI]

    . Bear Mountain, N.Y., March 28-301976. Hudson River Environmen- tal Society, Inc. FISHERY BULLETIN: VOL

  5. SSC 50 mm collider dipole cryostat design

    SciTech Connect (OSTI)

    Nicol, T.H.

    1992-04-01

    The cryostat of a Superconducting Super Collider (SSC) dipole magnet consists of all magnet components except the magnet assembly itself. It serves to support the magnet accurately and reliably within the vacuum vessel, provide all required cryogenic piping, and to insulate the cold mass from heat radiated and conducted from the environment. It must function reliably during storage, shipping and handling, normal magnet operation, quenches, and seismic excitations, and must be manufacturable at low cost. The major components of the cryostat are the vacuum vessel, thermal shields, multilayer insulation system, cryogenic piping, interconnections, and suspension system. The overall design of a cryostat for superconducting accelerator magnets requires consideration of fluid flow, proper selection of materials for their thermal and structural performance at both ambient and operating temperature, and knowledge of the environment to which the magnets will be subjected over the course of their expected operating life. This paper describes the design of the current SSC dipole magnet cryostat and includes discussions on the structural and thermal considerations involved in the development of each of the major systems.

  6. p'/raws SOCETICS mm 'FEB 241987

    E-Print Network [OSTI]

    McLeod, Ian

    REVIEWERS OF THE JOURNAL OF WATER RESOURCES PLANNING AND MANAGEMENT 159 in Downloaded 29 Jul 2010 to 129.100.76.58. Redistribution subject to ASCE license or copyright. Visit #12;#12;#12;#12;#12;#12;#12;#12;#12;#12;#12;#12;#12;#12;

  7. ARM - Campaign Instrument - 5mm-mwr

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Homesum_a_epg0_fpd_mmcf_m.xls" ,"Available from WebQuantity of NaturalDukeWakefieldSulfateSciTechtail.TheoryTuesday, August 10, 20102016StudyCHAPS:

  8. 20% (AM1.5) efficiency GaAs solar cells on sub-mm grain-size poly-Ge and its transition to low-cost substrates

    SciTech Connect (OSTI)

    Venkatasubramanian, R.; O`Quinn, B.C.; Siivola, E.; Keyes, B.; Ahrenkiel, R.

    1997-12-31

    Some of the key material and device issues related to the development of GaAs solar cells on poly-Ge substrates, including the dark-current reduction mechanism with an undoped spacer at the p{sup +}-n depletion layer, are discussed. Device-structure optimization studies that have led the authors to achieve an AM1.5 efficiency of {approximately}20% for a 4-cm{sup 2}-area GaAs cell on sub-mm grain-size poly-Ge and an efficiency of {approximately}21% for a 0.25-cm{sup 2}-area cell are presented. This successful demonstration of high-efficiency GaAs cells on sub-mm grain-size poly-Ge substrates have motivated us to consider the development of high-quality GaAs materials on significantly lower-cost substrates such as glass and moly foils. To date, the authors have achieved a best minority-carrier lifetime of 0.41 nsec in an n-GaAs thin-film on moly. The role of Group-VI dopant in the possible passivation of grain-boundaries in poly-GaAs is discussed. Development of PV-quality GaAs material, with minority-carrier lifetime of 1 to 2 nsec, on los-cost moly foils can significantly impact both the terrestrial and the space PV applications.

  9. Els UK Job: CDI Ch06-I047172 13-11-2007 11:15a.m. Page:245 Trim:165240MM Float:Top/Bot TS: Integra, India Fonts: Palatino & Helvetica 9/11 Margins:Top:4PC Gutter:5PC T. W:30PC open recto 1 Color 49 Lines

    E-Print Network [OSTI]

    Oren, Shmuel S.

    Els UK Job: CDI Ch06-I047172 13-11-2007 11:15a.m. Page:245 Trim:165×240MM Float:Top/Bot TS: Integra: CDI Ch06-I047172 13-11-2007 11:15a.m. Page:246 Trim:165×240MM Float:Top/Bot TS: Integra, India Fonts

  10. Complete 2mm Spectral Line Survey (130-170 GHz) of Sgr B2N, Sgr B2OH, IRC +10 216, Orion (KL), Orion-S, W51M, and W3(IRS5)

    E-Print Network [OSTI]

    Anthony. J. Remijan; Diane P. Leigh; A. J. Markwick-Kemper; B. E. Turner

    2008-02-15

    We report a complete 2mm spectral line survey (130-170 GHz) taken with the NRAO 12m Telescope between 1993 and 1995 toward the following sources: Sgr B2N, Sgr B2OH, IRC +10 216, Orion (KL), Orion-S, W51M, and W3(IRS5). Until very recently, this project was entirely the work of B. E. Turner. He wrote the original proposal, given below without changes or updates, and did all of the observing. B.E. Turner has fallen seriously ill and can no longer continue to work on the analysis of these data. The notes that follow the proposal give further information about the project and important information for users of these data. The data are distributed using the Spectral Line Search Engine (SLiSE) developed by A. J. Remijan and M. J. Remijan. SLiSE is a data display tool that will contain all the fully reduced and calibrated archived data taken as part of this 2mm survey. SLiSE is fast, easy to use, and contains the necessary functionality to display the data taken from spectral line searches. For example, SLiSE contains functions to overlay possible molecule identifications based on a current line catalog as well as overlaying H and He recombination lines. It is a Java-based applet, so it is platform independent and easily accessed online. The only caveat is that SLiSE was built using Java 1.5, so an update to the user's Java may be necessary. We request users of these data to give B.E. Turner and this work the appropriate citation and credit.

  11. Item # Value Description Manufacturer Manufacturer Part # Vendor Vendor Part Number Layout Part Ref Qty 1 POWER 3pin 2mm right angle connector Hirose Electronic Co. Ltd. DF3-3P-2DS Digikey H2106-ND J1 1

    E-Print Network [OSTI]

    Virginia Tech

    Qty 1 POWER 3pin 2mm right angle connector Hirose Electronic Co. Ltd. DF3-3P-2DS Digikey H2106-ND J1 1 2 SER A 3pin 2mm right angle connector Hirose Electronic Co. Ltd. DF3-3P-2DS Digikey H2106-ND J2 1 3 SER B 3pin 2mm right angle connector Hirose Electronic Co. Ltd. DF3-3P-2DS Digikey H2106-ND J3 1 4 SER

  12. Noncommutativity from the string perspective: modification of gravity at a mm without mm sized extra dimensions

    E-Print Network [OSTI]

    Steven Abel; Chong-Sun Chu; Mark Goodsell

    2006-09-27

    We explore how the IR pathologies of noncommutative field theory are resolved when the theory is realized as open strings in background B-fields: essentially, since the IR singularities are induced by UV/IR mixing, string theory brings them under control in much the same way as it does the UV singularities. We show that at intermediate scales (where the Seiberg-Witten limit is a good approximation) the theory reproduces the noncommutative field theory with all the (un)usual features such as UV/IR mixing, but that outside this regime, in the deep infra-red, the theory flows continuously to the commutative theory and normal Wilsonian behaviour is restored. The resulting low energy physics resembles normal commutative physics, but with additional suppressed Lorentz violating operators. We also show that the phenomenon of UV/IR mixing occurs for the graviton as well, with the result that, in configurations where Planck's constant receives a significant one-loop correction (for example brane-induced gravity), the distance scale below which gravity becomes non-Newtonian can be much greater than any compact dimensions.

  13. Coupling MM5 with LSM1: Development, Testing, and Application - MM5_workshop

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Homesum_a_epg0_fpd_mmcf_m.xls" ,"Available from WebQuantityBonneville Power Administration would like submit the followingConcentratingPortalCoolCoronaryCosts Associated4-Year/%2A

  14. Item # Value Description Manufacturer Manufacturer Part # Vendor Vendor Part Number Cost Layout Part Ref Qty 1 POWER 2pin 2mm right angle connector Hirose Electronic Co. Ltd. DF3-2P-2DS Digikey H2105-ND $0.18 J1 1

    E-Print Network [OSTI]

    Virginia Tech

    Backup Battery Circuit Diode D1 1 18 POWER LED 0603 SM LEDs (Red) Lite-On Trading USA, Inc. LTST-C190KRKT Part Ref Qty 1 POWER 2pin 2mm right angle connector Hirose Electronic Co. Ltd. DF3-2P-2DS Digikey H2105 SM (Battery Backup Circuit) R1 1 8 100 Ohm Resistor 0402 SM (Red,Orange, Green LEDs) R2, R3, R4 3 9

  15. A 76GHz PLL for mm-wave imaging applications

    E-Print Network [OSTI]

    Nguyen, Khoa M.

    A 76 GHz phase-locked loop (PLL) was designed in 0.13 ?m IBM BiCMOS8HP technology with the intended application of millimeter-wave imaging. The PLL has a type II second order loop filter. The voltage-controlled oscillator ...

  16. Discrimination Report: ESTCP UXO Discrimination Study, ESTCP Project #MM-0437

    E-Print Network [OSTI]

    Gasperikova, Erika; Smith, J. Torquil; Morrison, H. Frank; Becker, Alex

    2007-01-01

    UXO Detection and Discrimination: Partners in EnvironmentalDISCRIMINATION . .and characterization/ discrimination, and (2) the cued mode.

  17. A mm-scale aeroelastic oscillation-based anemometer

    E-Print Network [OSTI]

    McKay, Ian Salmon

    2012-01-01

    The flutter of a thin filament can provide a good indication of fluid velocity at small scales. By combining a 'fishtail'-shaped filament's aeroelastic and vortex-forced flutter modes, its oscillation frequency can be ...

  18. A mm-Scale Aeroelastic Oscillation-Based Anemometer

    E-Print Network [OSTI]

    McKay, Ian

    By combining the aeroelastic and vortex-forced flutter modes of a thin plastic strip, its oscillation frequency can be confined to scale monotonically with fluid velocity. This principle has been used to produce a low-cost, ...

  19. DESIGN OF 15 mm COLLARS FOR SSC DIPOLE MAGNETS

    E-Print Network [OSTI]

    Peters, C.

    2010-01-01

    layer. The Preliminary Design Criteria It will be helpful atand preliminary design criteria. Finite element analysisto meet the suggested design criteria. Three designs are

  20. Trim: 247mm 174mm Top: 14.762mm Gutter: 23.198mm CUUK2786-26 CUUK2786/Tong 978 1 107 04172 1 December 26, 2014 12:51

    E-Print Network [OSTI]

    Utrecht, Universiteit

    , as long as the wavelength of the waves is very much less than their path length, the ray approximation, T is the travel time, and ds is an increment along the ray path. Obtaining models of the solar or terrestrial wave construct images of a body's interior using seismic waves ­ is an inverse problem; that is, our goal

  1. Dimensions are shown in inch (mm ) Dimensions subject to change

    E-Print Network [OSTI]

    Berns, Hans-Gerd

    at 40°C, 93% RH SALT MIST RESISTANCE: 96 hours Materials COVER & BASE: Thermoplastic PPS ACTUATOR: PA Thermoplastic KNOB: Thermoplastic MOVABLE CONTACTS: Brass, gold or silver plated. STATIONARY CONTACTS: Brass

  2. NaCoMM-2003 Sponsors National Advisory Committee

    E-Print Network [OSTI]

    Saha, Subir Kumar

    SuwamaB. Torgal, Tripthi K. And N. K. Nagar TheStudy Of Five-Bar Mechanism With Variable Topology Mechanismsand Manipulators Optimal Design Of Mechanism For Stirrup Making Machine -A Computer Approach V SandijmnBandyopadhyayAnd Ashitava Gbosal Simulation Of SoftwareFor Four-Bar Function GeneratorMechanism

  3. Microsoft Word - MM5_LSM_JGR.doc

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Homesum_a_epg0_fpd_mmcf_m.xls" ,"Available from WebQuantityBonneville Power Administration wouldMass map shines light on77 PAGE OF PAGESpersonal CERTIFIEDPUB-3140September0 3.Impact of

  4. Posters Surface Flux Intercomparison Between the MM5 Model

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Homesum_a_epg0_fpd_mmcf_m.xls" ,"Available from WebQuantityBonneville Power Administration wouldMass mapSpeedingProgram Guidelines This document outlines the majorL.Posters955

  5. 40 MM Grenade Launcher Qualification Requirements at Department of Energy

    Broader source: Energy.gov (indexed) [DOE]

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Homesum_a_epg0_fpd_mmcf_m.xls" ,"Available from WebQuantity of Natural GasAdjustmentsShirleyEnergyTher i n c i p a l De p u t y A s s iof1 of 8 2 of 8of|under23-25,Chairman

  6. THE CM-, MM-, AND SUB-MM-WAVE SPECTRUM OF ALLYL ISOCYANIDE AND RADIOASTRONOMICAL OBSERVATIONS IN ORION KL AND THE SgrB2 LINE SURVEYS

    SciTech Connect (OSTI)

    Haykal, I.; Margulès, L.; Huet, T. R.; Motyienko, R. A.; Écija, P.; Cocinero, E. J.; Basterretxea, F.; Fernández, J. A.; Castaño, F.; Guillemin, J. C.; Tercero, B.; Cernicharo, J.

    2013-11-10

    Organic isocyanides have an interesting astrochemistry and some of these molecules have been detected in the interstellar medium (ISM). However, rotational spectral data for this class of compounds are still scarce. We provide laboratory spectra of the four-carbon allyl isocyanide covering the full microwave region, thus allowing a potential astrophysical identification in the ISM. We assigned the rotational spectrum of the two cis (synperiplanar) and gauche (anticlinal) conformations of allyl isocyanide in the centimeter-wave region (4-18 GHz), resolved its {sup 14}N nuclear quadrupole coupling (NQC) hyperfine structure, and extended the measurements into the millimeter and submillimeter-wave (150-900 GHz) ranges for the title compound. Rotational constants for all the monosubstituted {sup 13}C and {sup 15}N isotopologues are additionally provided. Laboratory observations are supplemented with initial radioastronomical observations. Following analysis of an extensive dataset (>11000 rotational transitions), accurate ground-state molecular parameters are reported for the cis and gauche conformations of the molecule, including rotational constants, NQC parameters, and centrifugal distortion terms up to octic contributions. Molecular parameters have also been obtained for the two first excited states of the cis conformation, with a dataset of more than 3300 lines. The isotopic data allowed determining substitution and effective structures for the title compound. We did not detect allyl isocyanide either in the IRAM 30 m line survey of Orion KL or in the PRIMOS survey toward SgrB2. Nevertheless, we provided an upper limit to its column density in Orion KL.

  7. Trim size: 189mm x 246mm Tedesco c07.tex V3 -10/01/2014 2:16 P.M. Page 123 Remote sensing

    E-Print Network [OSTI]

    Raup, Bruce H.

    of Colorado, Boulder, USA 2Norwegian Water Resources and Energy Directorate, Oslo, Norway 3University accuracy over large regions in a short time. New sensors will be coming online soon that will continue, in the form of snow, avalanches and wind-blown snow, and ablation, which occurs principally through melt

  8. A MOLECULAR LINE SURVEY OF THE CARBON-RICH PROTOPLANETARY NEBULA AFGL 2688 IN THE 3 mm AND 1.3 mm WINDOWS

    SciTech Connect (OSTI)

    Zhang Yong; Kwok, Sun; Nakashima, Jun-ichi; Chau, Wayne [Department of Physics, University of Hong Kong, Pokfulam Road, Hong Kong (Hong Kong); Dinh-V-Trung, E-mail: zhangy96@hku.hk, E-mail: sunkwok@hku.hk, E-mail: junichi@hku.hk, E-mail: dvtrung@iop.vast.ac.vn [Institute of Physics, Vietnam Academy of Science and Technology, 10 DaoTan Street, BaDinh, Hanoi (Viet Nam)

    2013-08-10

    We present a spectral line survey of the protoplanetary nebula (PPN) AFGL 2688 in the frequency ranges of 71-111 GHz, 157-160 GHz, and 218-267 GHz using the Arizona Radio Observatory 12 m telescope and the Heinrich Hertz Submillimeter Telescope. A total of 143 individual spectral features associated with 32 different molecular species and isotopologues were identified. The molecules C{sub 3}H, CH{sub 3}CN, H{sub 2}CO, H{sub 2}CS, and HCO{sup +} were detected for the first time in this object. By comparing the integrated line strengths of different transitions, we are able to determine the rotation temperatures, column densities, and fractional abundances of the detected molecules. The C, O, and N isotopic ratios in AFGL 2688 are compared with those in IRC+10216 and the Sun, and were found to be consistent with stellar nucleosynthesis theory. Through comparisons of molecular line strengths in asymptotic giant branch stars, PPNs, and planetary nebulae, we discuss the evolution in circumstellar chemistry in the late stages of evolution.

  9. Biological effects in unirradiated human tissue induced by radiation damage up to 1 mm away

    E-Print Network [OSTI]

    Brenner, David Jonathan

    in extrapolating radiation risk estimates from epidemi- ologically accessible doses down to very low doses where) and for assessing the risk from a low-dose exposure to a carcinogen such as ionizing radiation, where only a small, New York, NY 10032; Radiation Biology Laboratory, Research and Environmental Surveillance, Radiation

  10. Assessing the Performance of 5mm White LED Light Sources for Developing-Country Applications

    E-Print Network [OSTI]

    Mills, Evan

    2007-01-01

    lamp. Off-grid lighting products using the poorer LEDs wouldLED products encountered in the market by firms designing and assembling complete lightingLED) light sources have recently attained levels of efficiency and cost that allow them to compete with fluorescent lighting

  11. MM@MMaking Maths at Manchester General Course Information for the 2013 event.

    E-Print Network [OSTI]

    Glendinning, Paul

    walk away from the Alan Turing (Mathematics) building. Students will have their own room, with working minutes. There is a multi-storey car park next door to the Alan Turing building. A map and detailed

  12. Student Name: ______________________________ Birthdate (MM/DD/YY): ____________ PART I SCREENING: Please answer the following questions

    E-Print Network [OSTI]

    Faso Burundi Cambodia Cameroon Cape Verde Central African Republic Chad China Colombia Comoros Congo

  13. Particle Image Velocimetry Measurements and Analysis of Bypass Data for a Scaled 6mm Gap

    SciTech Connect (OSTI)

    J.R. Wolf; T.E. Conder; R.R. Schultz

    2012-09-01

    The purpose of the fluid dynamics experiments in the MIR (Matched Index of-Refraction) flow system at Idaho National Laboratory (INL) is to develop benchmark databases for the assessment of Computational Fluid Dynamics (CFD) solutions of the momentum equations, scalar mixing, and turbulence models for the flow ratios between coolant channels and bypass gaps in the interstitial regions of typical prismatic standard fuel element (SFE) or upper reflector block geometries of typical Modular High-temperature Gas-cooled Reactors (MHTGR) in the limiting case of negligible buoyancy and constant fluid properties. The experiments will use optical techniques, primarily particle image velocimetry (PIV) in the INL Matched Index of Refraction (MIR) flow system.

  14. The off-axis jet structure in Mrk 501 at mm-wavelengths

    E-Print Network [OSTI]

    Shoko Koyama; Motoki Kino; Marcello Giroletti; Akihiro Doi; Hiroshi Nagai; Kazuhiro Hada; Kotaro Niinuma; Monica Orienti; Gabriele Giovannini; Eduardo Ros; Tuomas Savolainen; Miguel A. Pérez-Torres; Thomas P. Krichbaum

    2015-05-17

    We present results from 43 GHz (VLBA, six epochs from 2012.2 to 2013.2) and 86 GHz (GMVA, one epoch in 2012.4) observations toward the basis of the jet in the TeV Blazar Mrk 501. The 43-GHz data analysis reveals a new feature located northeast of the radio core, with a flux density of several tens of mJy, perpendicularly to the jet axis. The 86-GHz image shows the jet feature located 0.75 mas southeast of the radio core, which is consistent with the previous result. The location of Gaussian model for 0.75 mas feature does not coincide with those for the jets in the 43-GHz image, however, a distribution of emission is found. We also discuss the spectral indices of the core, the northeast feature, and the jet feature between 43 GHz and 86 GHz, which show flat-to-steep, steep, and flat-to-invert, respectively.

  15. An ATCA Survey of Sagittarius~B2 at 7~mm: Chemical Complexity Meets Broadband Interferometry

    E-Print Network [OSTI]

    Corby, Joanna F; Cunningham, Maria R; Menten, Karl M; Belloche, Arnaud; Schwab, Frederic R; Walsh, Andrew J; Balnozan, Egon; Bronfman, Leonardo; Lo, Nadia; Remijan, Anthony J

    2015-01-01

    We present a 30 - 50 GHz survey of Sagittarius B2(N) conducted with the Australia Telescope Compact Array (ATCA) with 5 - 10 arcsec resolution. This work releases the survey data and demonstrates the utility of scripts that perform automated spectral line fitting on broadband line data. We describe the line-fitting procedure, evaluate the performance of the method, and provide access to all data and scripts. The scripts are used to characterize the spectra at the positions of three HII regions, each with recombination line emission and molecular line absorption. Towards the most line-dense of the three regions characterised in this work, we detect ~500 spectral line components of which ~90 per cent are confidently assigned to H and He recombination lines and to 53 molecular species and their isotopologues. The data reveal extremely subthermally excited molecular gas absorbing against the continuum background at two primary velocity components. Based on the line radiation over the full spectra, the molecular a...

  16. SPECTROSCOPIE DES ONDES DE 1 A 5 mm (1) Par WALTER GORDY,

    E-Print Network [OSTI]

    Boyer, Edmond

    'effectua,it la transition dont j'ai parlé plus haut, Loubser et Townes [3] détectèrent le rayon- nement des'atténuation de cer- taines substances à des fréquences bien déterminées. Le klystron a beaucoup d'avantages sur

  17. rspb.royalsocietypublishing.org Cite this article: Turcotte MM, Davies TJ,

    E-Print Network [OSTI]

    Dhindsa, Rajinder

    . Proc. R. Soc. B 281: 20140555. http://dx.doi.org/10.1098/rspb.2014.0555 Received: 6 March 2014 Accepted://dx.doi.org/10.1098/rspb.2014.0555 or via http://rspb.royalsocietypublishing.org. Macroecological

  18. The Flare Activity of SgrA*; New Coordinated mm to X-Ray Observations

    E-Print Network [OSTI]

    A. Eckart; F. K. Baganoff; R. Schoedel; M. Morris; R. Genzel; G. C. Bower; D. Marrone; J. M. Moran; T. Viehmann; M. W. Bautz; W. N. Brandt; G. P. Garmire; T. Ott; S. Trippe; G. R. Ricker; C. Straubmeier; D. A. Roberts; F. Yusef-Zadeh; J. H. Zhao; R. Rao

    2005-12-16

    We report new simultaneous near-infrared/sub-millimeter/X-ray observations of the SgrA* counterpart associated with the massive 3-4x10**6 solar mass black hole at the Galactic Center. The main aim is to investigate the physical processes responsible for the variable emission from SgrA*. The observations have been carried out using the NACO adaptive optics (AO) instrument at the European Southern Observatory's Very Large Telescope and the ACIS-I instrument aboard the Chandra X-ray Observatory as well as the Submillimeter Array SMA on Mauna Kea, Hawaii, and the Very Large Array in New Mexico. We detected one moderately bright flare event in the X-ray domain and 5 events at infrared wavelengths.

  19. Scavenging Elemental Sb Through Addition of NbSb to Mm0.9Fe3...

    Office of Scientific and Technical Information (OSTI)

    Energy Sciences (SC-22) Country of Publication: United States Language: English Subject: solar (thermal), phonons, thermal conductivity, thermoelectric, mechanical behavior,...

  20. G6943y: Myths and Methods in Modeling (M&M's in M)

    E-Print Network [OSTI]

    Spiegelman, Marc W.

    favourite language here) , 2nd Edition (Press et al., 1992) is a useful reference. Other useful background methods of data analysis by providing a fundamental set of quantitative tools that would benefit all earth will illustrate the fundamental behavior of the most commonly occurring equa- tions and demonstrate how to choose

  1. Ferrite-Cored Solenoidal Induction Coil Sensor for BUD (MM-1667)

    E-Print Network [OSTI]

    Morrison, F.

    2012-01-01

    simple measurements with a spectrum analyzer to estimate thethis experiment we used the spectrum analyzer to measure the

  2. Vibrational Spectra of Water Solutions of Azoles from QM/MM Calculations: Effects of Solvation

    E-Print Network [OSTI]

    Guidoni, Leonardo

    the decomposition of the vibrational density of states of the gas phase and solution dynamics. The calculated shifts the structural and dynamical aspects of water solutions. X-ray as well as neutron diffraction are the main source and electronic structure of the molecule.1 We expect therefore that also its vibrational properties could

  3. Ab initio simulations of two-dimensional electronic spectra: The SOS//QM/MM approach

    E-Print Network [OSTI]

    Rivalta, I; Nenov, A; Cerullo, G; Mukamel, S; Garavelli, M; Garavelli, M

    2013-01-01

    calculations. Conclusions Two-dimensional electronic spectroscopy holds great potential for studying structure, dynamics,

  4. Electronic Properties of Disordered Organic Semiconductors via QM/MM Simulations

    E-Print Network [OSTI]

    Difley, Seth

    Organic semiconductors (OSCs) have recently received significant attention for their potential use in photovoltaic, light emitting diode, and field effect transistor devices. Part of the appeal of OSCs is the disordered, ...

  5. TITLE: AUTHOR(S) SUBMITTED TO: Mm EVOLUTIO:l C: S!LICIC

    Office of Scientific and Technical Information (OSTI)

    ?bul are vesicular ase they ar cole.:j nc;trssl:IIt, C,IIJC,- ing vapor saturation of the residual liquid. Direct rnixi:':; of rrlfic ariisilicic liquids is...

  6. Powering mm-Size Wireless Implants for Brain-Machine Interfaces

    E-Print Network [OSTI]

    Mark, Michael

    2011-01-01

    be another way of trading input power for rectificationbe chosen, trading off available power for a more efficientTrading-off channel loss for increased transmit power as

  7. UNIVERSIT`A DEGLI STUDI DI PERUGIA Facolt`a di Scienze MM. FF. e NN.

    E-Print Network [OSTI]

    Filippucci, Roberta

    gravemente non solo sul comportamento ma anche sulla fisiologia. Si considerano 12560 balene che vivono nell

  8. Laser amplifier based on a neodymium glass rod 150 mm in diameter

    SciTech Connect (OSTI)

    Shaykin, A A; Fokin, A P; Soloviev, A A; Kuzmin, A A; Shaikin, I A; Burdonov, K F; Khazanov, E A [Institute of Applied Physics, Russian Academy of Sciences, Nizhnii Novgorod (Russian Federation); Charukhchev, A V [Public Limited Company "Scientific research Institute for Optoelectronic Instrument Engineering", Leningrad region (Russian Federation)

    2014-05-30

    A unique large-aperture neodymium glass rod amplifier is experimentally studied. The small-signal gain distribution is measured at different pump energies. The aperture-averaged gain is found to be 2.3. The stored energy (500 J), the maximum possible pump pulse repetition rate, and the depolarisation in a single pulse and in a series of pulses with a repetition rate of one pulse per five minutes are calculated based on the investigations performed. It is shown that the use of this amplifier at the exit of the existing laser can increase the output pulse energy from 300 to 600 J. (lasers)

  9. Injection-locked composite lasers for mm-wave modulation : LDRD 117819 final report.

    SciTech Connect (OSTI)

    Wendt, Joel Robert; Vawter, Gregory Allen; Raring, James; Tauke-Pedretti, Anna; Alford, Charles Fred; Skogen, Erik J.; Chow, Weng Wah; Cajas, Florante G.; Overberg, Mark E.; Torres, David L.; Peake, Gregory Merwin

    2010-09-01

    This report summarizes a 3-year LDRD program at Sandia National Laboratories exploring mutual injection locking of composite-cavity lasers for enhanced modulation responses. The program focused on developing a fundamental understanding of the frequency enhancement previously demonstrated for optically injection locked lasers. This was then applied to the development of a theoretical description of strongly coupled laser microsystems. This understanding was validated experimentally with a novel 'photonic lab bench on a chip'.

  10. Small object transporter. [Patent: for objects 0. 01 to 2. 00 mm dia

    DOE Patents [OSTI]

    Winkler, M.A.

    1980-05-21

    The disclosure relates to a small object transporter. Gas is passed through a conduit having a venturi. Small objects are picked up at a first location by a pickup tube in communication with the venturi and are forced out one end of the conduit at a desired second location.

  11. HighFidelity Rapid Prototyping of 300mm Fabs through Discrete Event System Modeling #

    E-Print Network [OSTI]

    Reveliotis, Spiridon "Spyros"

    manufacturing industry has been driven by continuous technological advancement of the underlying production processes. Yet, as the industry matures, mere technology development is no longer su#cient. The e#ective deployment and exploitation of the system production capacity and operational capability become crit­ ical

  12. 0.5mm Pitch Board to Board Connector DF17 Series

    E-Print Network [OSTI]

    developed a new connector structure utilizing its unique technology, and greatly enhanced the resistance in a BOX structure and has also enhanced shock-proof, pinch-proof and scoop-proof performance. In addition

  13. SubstrateSubstrate Commercially available high density -alumina plate (14x14 mm2)

    E-Print Network [OSTI]

    Azad, Abdul-Majeed

    440 450 460 470 480 490 500 510 520 530 540 OHM SubstrateSubstrate Commercially available high followed by oxidation in a well-defined pO2 regime near the M-MOx proximity line by a suitable buffer gas Model. Fig. 4. Thermodynamic criteria for several M/MOx coexistence and practical pO2 regimes for phase

  14. Assessing the Performance of 5mm White LED Light Sources for Developing-Country Applications

    E-Print Network [OSTI]

    Mills, Evan

    2007-01-01

    with fluorescent lighting for off-grid applications in theProject includes an Off-Grid Lighting Technology Assessmentand the market success of off-grid lighting solutions for

  15. Hans Peter Schwefel Wireless Networks III, Fall 2005: MM3, Wireless Services

    E-Print Network [OSTI]

    Schwefel, Hans-Peter

    in wireless settings 3. Video Streaming · Encoding and tranmission principles, buffering issues · Enhancements

  16. Pulling of 3 mm diameter AlSb rods by micro-pulling down method

    E-Print Network [OSTI]

    Bourret-Courchesne Ph.D., Edith

    2009-01-01

    Sb) and AlSb crystal zirconia were expected as crucibles,crucible shape with zirconia. Page 3/10 Fig 1 : vitreous

  17. Cryostat design for the Superconducting Super Collider 50mm aperture dipole magnet

    SciTech Connect (OSTI)

    Nicol, T.H. ); Tsavalas, Y.P. . Medical Systems)

    1990-09-01

    The cryostat of an SSC dipole magnet consists of all magnet components except the cold mass assembly. It serves to support the cold mass accurately and reliably within the vacuum vessel, provide all required cryogenic piping, and to insulate the cold mass from heat radiated and conducted from the environment. It must function reliably during storage, shipping and handling, normal magnet operation, quenches, and seismic excitations and must be manufacturable at low cost. The major components of the cryostat are the vacuum vessel, thermal shields, multilayer insulation (MLI) system, cryogenic piping, interconnections, and suspension system. The overall design of a cryostat for superconducting accelerator magnets requires consideration of fluid flow, proper selection of materials for their thermal and structural performance at both ambient and operating temperature, and knowledge of the environment to which the magnets will be subjected over the course their 25 year expected life. This paper describes the design of the current SSC collider dipole magnet cryostat and includes discussions on the thermal, structural, and dynamic considerations involved in the development of each of the major systems. 7 refs., 1 fig., 2 tabs.

  18. Exploring the Multidimensional Free Energy Surface of Phosphoester Hydrolysis with Constrained QM/MM Dynamics

    E-Print Network [OSTI]

    Gerwert, Klaus

    , it is involved in the regulation of protein function, energy production, and other biochemical pathways in cellsExploring the Multidimensional Free Energy Surface of Phosphoester Hydrolysis with Constrained QM for Theoretical Studies, Schloss-Wolfsbrunnenweg 35, 69118 Heidelberg, Germany § Ruhr-Universitat Bochum

  19. rsif.royalsocietypublishing.org Cite this article: Ankarali MM, Sefati S,

    E-Print Network [OSTI]

    . The Roman text De Architectura by Vitruvius and the epon- ymous Vitruvian Man by Leornado Da Vinci exemplify applications. The ubiquity of bilateral (left­right, sagittal plane) symmetry in animals is genetically encoded by the fact that the left­right axis is unbiased either by gravity or by direction of movement. However

  20. Facolt di Scienze MM.FF.NN Corso di Laurea in informatica

    E-Print Network [OSTI]

    Lo Cigno, Renato Antonio

    della SSTHRESH; 2. tempo di trasferimento; 3. numero totale di pacchetti inviati in rete ed efficienza

  1. DESIGN AND PERFORMANCE OF 40 mm, 6.5 T, COLLARED, COLD-IRON MODEL MAGNETS

    E-Print Network [OSTI]

    Peters, C.

    2010-01-01

    i. J Cu to S.C. , i.6S' keystone Outer Jo strands of 0.0255I.S Cu to S.C. , i.24' keystone Fig. i shows the aluminum

  2. Powering mm-Size Wireless Implants for Brain-Machine Interfaces

    E-Print Network [OSTI]

    Mark, Michael

    2011-01-01

    Interfaces . . . . . . . . . . . . . . . . . . . . . . . . . . . . .machine interfaces [Lebedev06] . . . . . . . . . . . . .rectifier interface . . . . . . . . . . . . . . . A half-

  3. MHK ISDB/Sensors/0.2 mm Rainfall (2m cable) Smart Sensor | Open Energy

    Open Energy Info (EERE)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Page on QA:QAsource History View NewTexas:Montezuma,Information MHK ISDB/Instruments/NortekMonitor ADCP

  4. Compression of 1-mm-thick M9763 cellular silicone foam under lateral

    Office of Scientific and Technical Information (OSTI)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Homesum_a_epg0_fpd_mmcf_m.xls" ,"Available from WebQuantity of NaturalDukeWakefieldSulfate Reducing BacteriaConnect Collider Tests ofO y (Journal Article)ethanollipolyticaconfinement

  5. Compression of 1-mm-thick M9763 cellular silicone foam under lateral

    Office of Scientific and Technical Information (OSTI)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Homesum_a_epg0_fpd_mmcf_m.xls" ,"Available from WebQuantity of NaturalDukeWakefieldSulfate Reducing BacteriaConnect Collider Tests ofO y (Journal

  6. 0.1 nm0.1 nm1 nm1 nm10 nm10 nm100 nm100 nm11 mm1010 mm100100 mm1 mm1 mm1 cm1 cm10 cm10 cm1 m1 m10 m10 m100 m100 m1 km1 kmWWAVELENGTHAVELENGTHWAVELENGTHWWAVELENGTHW 0.01K (-273C) 100K 5000K5000K5000K5000K5000K 30,000K 30,000,000K

    E-Print Network [OSTI]

    visible and invisible light from across the Cosmos SKA (Square Kilometre Array) SKA will be the world nuclear power ALMA E-ELT GAIAJWST XMM SKA sea level 690km 384,400km ALMA (Atacama Large Millimetre Array) ALMA is a giant array of 66 antennas observing at millimetre/submillimetre wavelengths. Location

  7. 1Il!11: m:mm:lli11I,111 Illili:llili!!ill,1ll ill ill!!ii111,111,111 mm; 206 THE HUMAN FACTOR HAS KNOCKED THREE TIMES

    E-Print Network [OSTI]

    Meyer, Bertrand

    ................................................................................................................................ THE HUMAN FACTOR HAS KNOCKED THREE TIMES Three books on the ergonomics of computing systems B. Meyer vanous names to it: the ergonomics of computing systems, the study of human factors, software psy style, evaluation of software quality, data base management systems, use o.f natural language and design

  8. 0.5 mm 1.5 mm Within the framework of fusion technology research and development, a neutron source has long been considered a key facility to perform irradiation tests

    E-Print Network [OSTI]

    McDonald, Kirk

    at populating materials engineering database ­ supporting DEMO reactor design and licensing. New Sorgentina - impinging on a hydride thin layer which is on-line D-T reloaded via ion implantation. Metal hydride hydride layer as DT enriched target Rotating wheel target to manage high heat flux Continuous online layer

  9. P1: aaa Trim: 174mm 247mm Top: 0.553in Gutter: 0.747in CUUK632-10 CUUK632-Watters ISBN: 978 0 521 76573 2 June 26, 2009 21:33

    E-Print Network [OSTI]

    Mege, Daniel

    76573 2 June 26, 2009 21:33 10 Fault populations Richard A. Schultz Geomechanics ­ Rock Fracture Group

  10. Yeast Genomic DNA Preparation from Spheroplasts 1. Resuspend with 50 mM Tris, 25 mM EDTA (pH 8) in 10X the spheroplast pellet volume.

    E-Print Network [OSTI]

    Aris, John P.

    ) in 10X the spheroplast pellet volume. 2. Immediately add 1/10 volume of 10% SDS. Mix. 3. Incubate 30 up pellets. Wash for at least 5 minutes at 25°C. 11. Centrifuge 10 minutes in SS-34 rotor at 10,000 rpm at 4°C. Discard supernatant. 12. Drain and dry pellets on bench. Dissolve each pellet completely

  11. Portable TXRF Spectrometer with 10{sup -11}g Detection Limit and Portable XRF Spectromicroscope with Sub-mm Spatial Resolution

    SciTech Connect (OSTI)

    Kunimura, Shinsuke; Hatakeyama, So; Sasaki, Nobuharu; Yamamoto, Takashi; Kawai, Jun

    2010-04-06

    A portable total reflection X-ray fluorescence (TXRF) spectrometer that we have developed is applied to trace elemental analysis of water solutions. Although a 5 W X-ray tube is used in the portable TXRF spectrometer, detection limits of several ppb are achieved for 3d transition metal elements and trace elements in a leaching solution of soils, a leaching solution of solder, and alcoholic beverages are detected. Portable X-ray fluorescence (XRF) spectromicroscopes with a 1 W X-ray tube and an 8 W X-ray tube are also presented. Using the portable XRF spectromicroscope with the 1 W X-ray tube, 93 ppm of Cr is detected with an about 700 {mu}m spatial resolution. Spatially resolved elemental analysis of a mug painted with blue, red, green, and white is performed using the two portable spectromicroscopes, and the difference in elemental composition at each paint is detected.

  12. RELATIVISTIC JETS FROM ACCRETION DISKS R.V.E. LOVELACE, P.R. GANDHI and M.M. ROMANOVA

    E-Print Network [OSTI]

    momentum and energy from the disk. Two main regimes have been discussed, hydro- magnetic jets, which have and, Poynting jets, where the mass flux is small and energy and angular momentum are carried The powerful jets observed from active galaxies and quasars are probably not hydro- magnetic outflows

  13. 1 M-M@0?t$N@0=--3 2 O"J,?t 11

    E-Print Network [OSTI]

    Sato, Atsushi

    + · · · + anZ = dZ. [ ¿ZL@] Nc1.2 $HDjM1.4 $h$j, a1Z + · · · + anZ = aZ a Z+ { 0 } ($?$@1 $D) B8:$9$k. $3 ai a1Z + · · · + anZ = aZ , a a1, . . . , an t . $h$C$Fd . B ja d. 0J¿e$h$j a = d k k. 1.7 a1

  14. CC UU RR RR II CC UU LL UU MM VV II TT AA EE Thursday, 25 September 2014

    E-Print Network [OSTI]

    Synthesis of nanomaterials such as nanoparticles, carbon nanotubes, graphene structures, metal oxide: 2007: Helmi Keskinen "Synthesis of nanoparticles and preparation of deposits by liquid flamme spray

  15. 1010 OPTICS LETTERS / Vol. 23, No. 13 / July 1, 1998 16-mm infrared generation by difference-frequency mixing

    E-Print Network [OSTI]

    Byer, Robert L.

    -tal Technol- ogy) were diced into 1-cm squares, stacked together, and put into a bonding furnace. The furnace- plied at 600 ± C, and the pressure in the furnace was maintained at 30 mTorr of H2. The furnace

  16. Temperature effects on the 1585 mm spectra of olivines and pyroxenes J. E. Bowey,1,2P

    E-Print Network [OSTI]

    Bowey, Janet

    and planetary nebulae (e.g. Waters et al. 1996; Cohen et al. 1999; Malfait et al. 1999; Sylvester et al. 1999 emission occurs at temperatures in the 50­100 K range (e.g. Sylvester et al. 1999). However, previous laboratory studies (e.g. Day 1976; Agladze et al. 1996; Henning & Mutschke 1997; Mennella et al. 1998) have

  17. Elements for the design of precision machine tools and their application to a prototype 450mm Si-wafer grinder

    E-Print Network [OSTI]

    Rothenhöfer, Gerald S. (Gerald Sven)

    2010-01-01

    Next generation precision machines will require ever more rigid elements to achieve the required machining tolerances. The presented work focuses on the application of ultra stiff servo-controllable kinematic couplings and ...

  18. Development of TQC01, a 90 mm Nb3 Sn Model Quadrupole for LHC Upgrade Based on SS Collar

    E-Print Network [OSTI]

    Bossert, R. C.

    2009-01-01

    A ) keys are inserted and hydraulic press load is released,coils and closed in a hydraulic press. Col- laring keys are

  19. [Km 100 to 1000 mM (17)] and to S. cerevisiae hexose transporters' apparent affinity for glucose

    E-Print Network [OSTI]

    Severson, David

    , and British Petroleum Technology Ventures (through the Energy Biosciences Institute) have submitted a patent

  20. Absence of correlation between Sry polymorphisms and XY sex reversal caused by the M.m. domesticus Y chromosome

    SciTech Connect (OSTI)

    Carlisle, C.; Nagamine, C.M. [Vanderbilt Univ., School of Medicine, Nashville, TN (United States)] [Vanderbilt Univ., School of Medicine, Nashville, TN (United States); Winkinig, H.; Weichenhan, D. [Medizinische Universitaet Zu Luebeck (Germany)] [Medizinische Universitaet Zu Luebeck (Germany)

    1996-04-01

    Mus musculus domesticus Y chromosomes (Y{sup DOM} Chrs) vary in their ability to induce testes in the strain C57BL/6J. In severe cases, XY females develop (XY{sup DOM} sex reversal). To identify the molecular basis for the sex reversal, a 2.7-kb region of Sry, the testis-determining gene, was sequenced from Y{sup DOM} Chrs linked to normal testis determination, transient sex reversal, and severe sex reversal. Four mutations were identified. However, no correlation exists between these mutations and severity of XY{sup DOM} sex reversal. RT-PCR identified Sry transcripts in XY{sup DOM} sex-reversed fetal gonads at 11 d.p.c., the age when Sry is hypothesized to function. In addition, no correlation exists between XY{sup DOM} sex reversal and copy numbers of pSx1, a Y-repetitive sequence whose deletion is linked to XY sex reversal. We conclude that SRY protein variants, blockade of Sry transcription, and deletion of pSx1 sequences are not the underlying causes of XY{sup DOM} sex reversal. 63 refs., 6 figs., 6 tabs.

  1. Stratus Cloud Structure from MM-Radar Transects and Satellite Images: Scaling Properties and Artifact Detection with Semi-...

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Homesum_a_epg0_fpd_mmcf_m.xls" ,"Available from WebQuantityBonneville Power AdministrationRobust,Field-effect Photovoltaics -7541C.3X-rays3 PreparedcordiallyGlobalHigh-LevelStructure from

  2. IdentIfIcacIn Mariposa diurna mediana (ala anterior: 24-28 mm). adulto de alas pardas, dorso con gruesos

    E-Print Network [OSTI]

    García-Barros, Enrique

    no interconectados, en los Picos de europa y su entorno (provincias de asturias, León y cantabria). estas zonas de provincia. núcleo occidental en asturias (amieva, Ponga y cabrales), León (Posada de Valdeón) y cantabria

  3. 190 2008 IEEE International Solid-State Circuits Conference ISSCC 2008 / SESSION 9 / mm-Wave & PHASED ARRAYS / 9.6

    E-Print Network [OSTI]

    Razavi, Behzad

    , and (3) a component shifted to -90GHz. Since the output currents of these mixers flow through load tanks of a single RF mixer and quadrature IF mixers suffers from an additional image introduced by the third of the RF mixer convolves the +90GHz harmonic with the signal spectrum at -60GHz, thus translating

  4. 12th IFToMM World Congress, Besancon, June 18-21, 2007 A Method to Determine the Motion of Overconstrained 6R-Mechanisms

    E-Print Network [OSTI]

    Nawratil, Georg

    -loop. The mechanism becomes overcon- strained, when the inverse kinematics yields infinitely many solutions. The Inverse Kinematics Problem A serial 6R-mechanism can be modeled as a kinematic chain with a fixed link of Overconstrained 6R-Mechanisms M. Pfurner M.L. Husty University Innsbruck, Institute for Basic Sciences

  5. Artificial neural network modeling of the spontaneous combustion occurring in the industrial-scale coal stockpiles with 10-18 mm coal grain sizes

    SciTech Connect (OSTI)

    Ozdeniz, A.H.; Yilmaz, N. [Selcuk University, Konya (Turkey). Dept. of Mining Engineering

    2009-07-01

    Companies consuming large amounts of coal should work with coal stocks in order to not face problems due to production delays. The industrial-scale stockpiles formed for the aforementioned reasons cause environmental problems and economic losses for the companies. This study was performed in a coal stock area of a large company in Konya, which uses large amounts of coal in its manufacturing units. The coal stockpile with 5 m width, 10 m length, 3 m height, and having 120 tons of weight was formed in the coal stock area of the company. The inner temperature data of the stockpile was recorded by 17 temperature sensors placed inside the stockpile at certain points. In order to achieve this goal, the electrical signal conversion of temperatures sensed by 17 temperature sensors placed in certain points inside the coal stockpile, the transfer of these electrical signals into computer media by using analog-digital conversion unit after applying necessary filtration and upgrading processes, and the record of these information into a database in particular time intervals are provided. Additionally, the data relating to the air temperature, air humidity, atmospheric pressure, wind velocity, and wind direction that are the parameters affecting the coal stockpile were also recorded. Afterwards, these measurement values were used for training and testing of an artificial neural network model. Comparison of the experimental and artificial neural network results, accuracy rates of training and testing were found to be 99.5% and 99.17%, respectively. It is shown that possible coal stockpile behavior with this artificial neural network model is powerfully estimated.

  6. Feasibility study for a 10 MM GPY fuel ethanol plant, Brady Hot Springs, Nevada. Volume II. Geothermal resource, agricultural feedstock, markets and economic viability

    SciTech Connect (OSTI)

    Not Available

    1980-09-01

    The issues of the geothermal resource at Brady's Hot Springs are dealt with: the prospective supply of feedstocks to the ethanol plant, the markets for the spent grain by-products of the plant, the storage, handling and transshipment requirements for the feedstocks and by-products from a rail siding facility at Fernley, the probable market for fuel ethanol in the region, and an assessment of the economic viability of the entire undertaking.

  7. Feasibility study for a 10-MM-GPY fuel ethanol plant, Brady Hot Springs, Nevada. Volume 1. Process and plant design

    SciTech Connect (OSTI)

    Not Available

    1980-09-01

    An investigation was performed to determine the technical and economic viability of constructing and operating a geothermally heated, biomass, motor fuel alcohol plant at Brady's Hot Springs. The results of the study are positive, showing that a plant of innovative, yet proven design can be built to adapt current commerical fermentation-distillation technology to the application of geothermal heat energy. The specific method of heat production from the Brady's Hot Spring wells has been successful for some time at an onion drying plant. Further development of the geothermal resource to add the capacity needed for an ethanol plant is found to be feasible for a plant sized to produce 10 million gallons of motor fuel grade ethanol per year. A very adequate supply of feedgrains is found to be available for use in the plant without impact on the local or regional feedgrain market. The effect of diverting supplies from the animal feedlots in Northern Nevada and California will be mitigated by the by-product output of high-protein feed supplements that the plant will produce. The plant will have a favorable impact on the local farming economies of Fallon, Lovelock, Winnemucca and Elko, Nevada. It will make a positive and significant socioeconomic contribution to Churchill County, providing direct employment for an additional 61 persons. Environmental impact will be negligible, involving mostly a moderate increase in local truck traffic and railroad siding activity. The report is presented in two volumes. Volume 1 deals with the technical design aspects of the plant. The second volume addresses the issue of expanded geothermal heat production at Brady's Hot Springs, goes into the details of feedstock supply economics, and looks at the markets for the plant's primary ethanol product, and the markets for its feed supplement by-products. The report concludes with an analysis of the economic viability of the proposed project.

  8. Plasma Physics Challenges of MMPlasma Physics Challenges of MM--toto--THz and High Power MicrowaveTHz and High Power Microwave

    E-Print Network [OSTI]

    of radio waves, confirming Maxwell's theory · 1917: Tesla proposed radio wave radar H. Hertz, Karlsrühe hardware enabled basic research in microwave spectroscopy, atmospheric science, radar, maser, and radio energy research Charged particle accelerators Atmospheric radar Radio astronomy Medical

  9. Total RNA From Yeast Using Glass Beads In advance, prepare 2 ml tubes containing 0.25 g acid washed glass beads (0.5 mm diameter) and

    E-Print Network [OSTI]

    Aris, John P.

    Total RNA From Yeast Using Glass Beads In advance, prepare 2 ml tubes containing 0.25 g acid washed. 1. Collect 5 OD600 units of yeast (e.g., 10 mls of OD600 = 0.5). Centrifuge for 5 minutes at 2000 different time points by centrifugation and store at -80°C. At step 6: collect exactly the same volume

  10. Combining quantum wavepacket ab initio molecular dynamics with QM/MM and QM/QM techniques: Implementation blending ONIOM and empirical

    E-Print Network [OSTI]

    Iyengar, Srinivasan S.

    : Implementation blending ONIOM and empirical valence bond theory Isaiah Sumner and Srinivasan S. Iyengara. All components of the methodology, namely, quantum dynamics and ONIOM molecular dynamics

  11. 5000 groove/mm multilayer-coated blazed grating with 33percent efficiency in the 3rd order in the EUV wavelength range

    SciTech Connect (OSTI)

    Advanced Light Source; Voronov, Dmitriy L.; Anderson, Erik; Cambie, Rossana; Salmassi, Farhad; Gullikson, Eric; Yashchuk, Valeriy; Padmore, Howard; Ahn, Minseung; Chang, Chih-Hao; Heilmann, Ralf; Schattenburg, Mark

    2009-07-07

    We report on recent progress in developing diffraction gratings which can potentially provide extremely high spectral resolution of 105-106 in the EUV and soft x-ray photon energy ranges. Such a grating was fabricated by deposition of a multilayer on a substrate which consists ofa 6-degree blazed grating with a high groove density. The fabrication of the substrate gratings was based on scanning interference lithography and anisotropic wet etch of silicon single crystals. The optimized fabrication process provided precise control of the grating periodicity, and the grating groove profile, together with very short anti-blazed facets, and near atomically smooth surface blazed facets. The blazed grating coated with 20 Mo/Si bilayers demonstrated a diffraction efficiency in the third order as high as 33percent at an incidence angle of 11? and wavelength of 14.18 nm.

  12. A Large System of 500 MHz Transient M.S. Atiya, J.S. Haggerty, M.M. Ito, C. Ng

    E-Print Network [OSTI]

    elements has often enriched our understanding of the devices generating the signals and fre­ quently the detector in both the barrel and endcap regions. A 1 Tesla solenoidal coil surrounds the entire detector

  13. eyeROBOT -Heterogeneous Robotic Platform for Real-time Computer Vision Mohit Modi (mm2675), Sravya Chinthalapati (sc2655), Shang Dang (sd687), Yunong Liu (yl2494)

    E-Print Network [OSTI]

    Afshari, Ehsan

    is a mobile robotic platform which can be driven based on the input commands provided over serial interface-software co-design including FPGA prototyping, High-Level Digital Synthesis (HLS), Embedded System Development Window FPGA Video Accelerator TX RX OpCode Velocity (MSB) Velocity (LSB) Radius (MSB) Radius (LSB) 1 Byte

  14. Multiscale QM/MM Molecular Dynamics Study on the First Steps of Guanine-Damage by Free Hydroxyl Radicals in Solution

    E-Print Network [OSTI]

    Abolfath, Ramin M; Rajnarayanam, R; Brabec, Thomas; Kodym, Reinhard; Papiez, Lech

    2012-01-01

    Understanding the damage of DNA bases from hydrogen abstraction by free OH radicals is of particular importance to reveal the effect of hydroxyl radicals produced by the secondary effect of radiation. Previous studies address the problem with truncated DNA bases as ab-initio quantum simulation required to study such electronic spin dependent processes are computationally expensive. Here, for the first time, we employ a multiscale and hybrid Quantum-Mechanical-Molecular-Mechanical simulation to study the interaction of OH radicals with guanine-deoxyribose-phosphate DNA molecular unit in the presence of water where all the water molecules and the deoxyribose-phosphate fragment are treated with the simplistic classical Molecular-Mechanical scheme. Our result illustrates that the presence of water strongly alters the hydrogen-abstraction reaction as the hydrogen bonding of OH radicals with water restricts the relative orientation of the OH-radicals with respective to the the DNA base (here guanine). This results ...

  15. J.A. Leenheer & M.M. Reddy, Annals of Environmental Science / 2008, Vol 2, 11-25 www.aes.northeastern.edu, ISSN 1939-2621 11

    E-Print Network [OSTI]

    , including the Green River Formation oil shale, which is well known as one the world's largest potential

  16. Investigation of surface inhomogeneity and estimation of the GOES skin temperature assimilation errors of the MM5 implied by the inhomogeneity over Houston metropolitan area 

    E-Print Network [OSTI]

    Han, Sang-Ok

    2005-11-01

    by about 25 %, thereby inducing the warmer (0.7 %) and drier (-1.0 %) PBL and the colder and moister PBL top induced by greater turbulent diffusivities. The 3-d application of the inhomogeneity parameterization indicated consistent results with the 1-d...

  17. IL DIRETTORE Visti i DD.MM. 4.10.2000 e 9.1.2001 concernenti la rideterminazione, l'aggiornamento

    E-Print Network [OSTI]

    Di Pillo, Gianni

    Dipartimento di Fisiologia e Farmacologia "Vittorio Erspamer" e la Fondazione "Enrico ed Enrica Sovena", con chemiopreventivi"; Vista la Delibera del Consiglio del Dipartimento di Fisiologia e Farmacologia "Vittorio Erspamer Fisiologia e Farmacologia "Vittorio Erspamer" ad attivare la procedura per il reclutamento di un ricercatore

  18. 1.1 0.2 were bound to the column and were eluted by 30 mM and 1 M HCI, respec-

    E-Print Network [OSTI]

    Boyer, Edmond

    infusion on postabsorp- tive glycemia in non insulin dependent diabetes mellitus (NIDDM). V Rigalleau previously reported a hyper- glycemic effect of a lipid infusion in the postabsorptive state in NIDD patients patients. Fifteen received a 180 min lipid infusion (')veiip20%'; 0.0155 mUkg/min) and 15 received saline

  19. Investigating the chemical and morphological evolution of GaAs capped InAs/InP quantum dots emitting at 1.5 mm using aberration-corrected

    E-Print Network [OSTI]

    Dunin-Borkowski, Rafal E.

    s t r a c t The emission wavelength of InAs quantum dots grown on InP has been shown to shiftInvestigating the chemical and morphological evolution of GaAs capped InAs/InP quantum dots microscopy A3. Metalorganic vapour-phase epitaxy A3. Quantum dots B2. Semiconducting III/V materials a b

  20. 23.2 A Modular 1mm3 Die-Stacked Sensing Platform With Optical Communication and Multi-Modal Energy

    E-Print Network [OSTI]

    Dutta, Prabal

    and synchronization. It also includes an ultra-low power PMU (Power Management Unit) with BOD (Brown-Out Detector ranges from 11nW in sleep mode up to ~40µW in active mode. A flexible PMU allows harvesting for perpetual

  1. horizontal de 60 cm de long, avec une tension de 100 200 volts et du papier Whatman No 3MM de 5 cul de

    E-Print Network [OSTI]

    Paris-Sud XI, Université de

    source, déposée à une extrémité, migrer environ jusqu'aux 2/3 de la longueur du papier. 147 Pm additionné même pour toutes les fractions de,1 /2 cm correspondant à la zone Sm - Pm - Nd. La raie de 121 ke carbone absorbant les p-, est (3 :1: 0,5)10-1 /P- de 14'Pm. C. Conclusion : Origine du rayonnement de 121

  2. Structural properties of free-standing 50 mm diameter GaN waferswith (101_0) orientation grown on LiAlO2

    SciTech Connect (OSTI)

    Jasinski, Jacek; Liliental-Weber, Zuzanna; Maruska, Herbert-Paul; Chai, Bruce H.; Hill, David W.; Chou, Mitch M.C.; Gallagher, John J.; Brown, Stephen

    2005-09-27

    (10{und 1}0) GaN wafers grown on (100) face of {gamma}-LiAlO{sub 2} were studied using transmission electron microscopy. Despite good lattice matching in this heteroepitaxial system, high densities of planar structural defects in the form of stacking faults on the basal plane and networks of boundaries located on prism planes inclined to the layer/substrate interface were present in these GaN layers. In addition, significant numbers of threading dislocations were observed. High-resolution electron microscopy indicates that stacking faults present on the basal plane in these layers are of low-energy intrinsic I1type. This is consistent with diffraction contrast experiments.

  3. Exploring the molecular chemistry and excitation in obscured luminous infrared galaxies: An ALMA mm-wave spectral scan of NGC 4418

    E-Print Network [OSTI]

    Costagliola, F; Muller, S; Martín, S; Aalto, S; Harada, N; van der Werf, P; Viti, S; Garcia-Burillo, S; Spaans, M

    2015-01-01

    We obtained an ALMA Cycle 0 spectral scan of the dusty LIRG NGC 4418, spanning a total of 70.7 GHz in bands 3, 6, and 7. We use a combined local thermal equilibrium (LTE) and non-LTE (NLTE) fit of the spectrum in order to identify the molecular species and derive column densities and excitation temperatures. We derive molecular abundances and compare them with other Galactic and extragalactic sources by means of a principal component analysis. We detect 317 emission lines from a total of 45 molecular species, including 15 isotopic substitutions and six vibrationally excited variants. Our LTE/NLTE fit find kinetic temperatures from 20 to 350 K, and densities between 10$^5$ and 10$^7$ cm$^{-3}$. The spectrum is dominated by vibrationally excited HC$_3$N, HCN, and HNC, with vibrational temperatures from 300 to 450 K. We find high abundances of HC$_3$N, SiO, H$_2$S, and c-HCCCH and a low CH$_3$OH abundance. A principal component analysis shows that NGC 4418 and Arp 220 share very similar molecular abundances and ...

  4. 5000 Groove/mm multilayer-coated blazed grating with 33% efficiency in the 3rd order in the EUV wavelength range

    E-Print Network [OSTI]

    Schattenburg, Mark Lee

    We report on recent progress in developing diffraction gratings which can potentially provide extremely high spectral resolution of 10[superscript 5]-10[superscript 6] in the EUV and soft x-ray photon energy ranges. Such ...

  5. The Ability of MM5 to Simulate Ice Clouds: Systematic Comparison between Simulated and Measured Fluxes and Lidar/Radar Profiles at the

    E-Print Network [OSTI]

    Protat, Alain

    -term meteorological measurements by active (radar and lidar) and passive (infrared and visible fluxes) remote sensing effect is governed primarily by the equi- librium between their albedo effect and their green- house

  6. JvMF:210x280mmKunde:RWE 13410/10/10005/01Produkt:energiewelt.de;Stromberg,,Dmmung"

    E-Print Network [OSTI]

    Falge, Eva

    feststellt, werden neue Techniken und Investitionschancen in Kohlen- dioxid-arme und erneuerbare Energien

  7. The sensitivity of the PSU-NCAR model (MM5) to cumulus parameterization in simulating the mesoscale environment associated with 2 June 1995 West Texas tornado outbreak 

    E-Print Network [OSTI]

    Han, Sang-Ok

    1998-01-01

    important role in producing tornadic supercedes. This study presents observational features of the event, performs model simulations with three disparate cumulus parameterization schemes, and does a careful comparison between the simulations and observations...

  8. Scavenging Elemental Sb Through Addition of NbSb to Mm0.9Fe3.5Co0.5S12

    Office of Scientific and Technical Information (OSTI)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Homesum_a_epg0_fpd_mmcf_m.xls" ,"Available from WebQuantity of NaturalDukeWakefieldSulfateSciTechtail. (Conference) | SciTechsaturated fractured rock (Journal(Journal

  9. Measurement of Boundary-Layer Temperature Profiles by a Scanning 5-MM Radiometer During the 1999 Winter NSA/AAO Radiometer Exp

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Homesum_a_epg0_fpd_mmcf_m.xls" ,"Available from WebQuantityBonneville Power Administration wouldMass map shines light on dark matter By SarahMODELING CLOUD1 H( 7 Be, 8Measurement

  10. STRENGTH AND PERMEABILITY TESTS ON ULTRA-LARGE STRIPA GRANITE CORE

    E-Print Network [OSTI]

    Thorpe, R.

    2009-01-01

    2-0.0598 mm 16-0.0241 mm 58.5 rns 0 em :C mm mnl mm ms dC 4mm mm mm ms dC mm mm mm mm rns 5-0.0697 mm 12-0.2679 mm 19-KPa mm mm ms em mm mm mm rns dC mm mm mm ms mm mm mm ms 6

  11. Els UK SOI Ch04-N52975 Trim:165MM240MM 5-9-2007 9:30p.m. Page:117 Float:Top/Bot TS: Integra, India Fonts: Times & Copperplate 32BC 10/12pt Margins:Top:4pc Gutter:5pc T.Area:29pcx43p9 open recto 1 Color 44 Lines

    E-Print Network [OSTI]

    Lieth, J. Heinrich

    for the fraction of water that ends up tied up in biomass. While transpiration cools the leaves, this flux) of the total water actually ends up as fresh matter (Raviv and Blom, 2001). The rest of the water is transpired and most of this water use is necessary as part of the plant's need to cool itself. The total amount

  12. Life Cycle Assessment of Pavements: A Critical Review of Existing Literature and Research

    E-Print Network [OSTI]

    Santero, Nicholas

    2010-01-01

    50 mm) | stone (150 mm) | fly ash + cement (650 mm) | sand (mm) | stone (150 mm) | fly ash + cement (350 mm) | sand (200160 mm) | stone (150 mm) | fly ash (350 mm) | sand (200 mm)

  13. BB UU LL GG AA RR II AA NN AA CC AA DD EE MM YY OO FF SS CC II EE NN CC EE SS IINNSSTTIITTUUTTEE OOFF IINNFFOORRMMAATTIIOONN AANNDD CCOOMMMMUUNNIICCAATTIIOONN TTEECCHHNNOOLLOOGGIIEESS

    E-Print Network [OSTI]

    Borissova, Daniela

    Library (ITIL) ­ essence development, open problems Abstract: This article aims to give an overview over the ITIL framework objective. It is going to explain the rapidly growing IT business needs which had caused the development of this library. We are also going to follow the ITIL evolution history and find the circumstances

  14. 400 2005 IEEE International Solid-State Circuits Conference 0-7803-8904-2/05/$20.00 2005 IEEE. ISSCC 2005 / SESSION 21 / TD: RF TRENDS: ABOVE-IC INTEGRATION AND MM-WAVE / 21.6

    E-Print Network [OSTI]

    Razavi, Behzad

    the receiver architecture. The circuit consists of a low-noise amplifier (LNA), quadrature mixers, and baseband the layout of the overall receiver more difficult. Approximating the folded microstrip by the lumped tank

  15. Friction Factor Measurement, Analysis, and Modeling for Flat-Plates with 12.15 mm Diameter Hole-Pattern, Tested with Air at Different Clearances, Inlet Pressures, and Pressure Ratios 

    E-Print Network [OSTI]

    Deva Asirvatham, Thanesh

    2011-02-22

    Friction factor data are important for better prediction of leakage and rotordynamic coefficients of gas annular seals. A flat-plate test rig is used to determine friction factor of hole-pattern/honeycomb flat-plate surfaces ...

  16. Product (a) Type (b) Time of Harvest Gear Code (c) Area of catch (d) Net Weight No. of Fish F/FR RD/GG/DR/FL/OT (mm/yy) (kg) (when RD, GG or DR)

    E-Print Network [OSTI]

    Product (a) Type (b) Time of Harvest Gear Code (c) Area of catch (d) Net Weight No. of Fish F/FR RD=Other (describe the type of product; ____________________.) (c): If the Gear Code is OT, describe the type of gear

  17. Domain patterning in lithium niobate using spontaneous backswitching R.G. Batchko*, G.D. Millerb, V. Ya. Shur', E. L. Rumyantsevc M.M. Fejer', and R.L. Byera

    E-Print Network [OSTI]

    Byer, Robert L.

    -1208 Clnstitute of Physics and Applied Mathematics, Ural State University, Ekaterinburg 620083, Russia ABSTRACT

  18. Ertek, G., Tun, M.M., Kurtaraner, E., Kebude, D., 2012, 'Insights into the Efficiencies of On-Shore Wind Turbines: A Data-Centric Analysis', INISTA 2012 Conference. July 2-4, 2012, Trabzon,

    E-Print Network [OSTI]

    Yanikoglu, Berrin

    -Shore Wind Turbines: A Data-Centric Analysis', INISTA 2012 Conference. July 2-4, 2012, Trabzon, Turkey://research.sabanciuniv.edu. Insights into the Efficiencies of On-Shore Wind Turbines: A Data-Centric Analysis Gürdal Ertek, Murat University Istanbul, Turkey Abstract--Literature on renewable energy alternative of wind turbines does

  19. 50-nm E-mode In[subscript 0.7]Ga[subscript 0.3]As PHEMTs on 100-mm InP substrate with f[subscript max] > 1 THz

    E-Print Network [OSTI]

    del Alamo, Jesus A.

    We have demonstrated 50-nm enhancement-mode (E-mode) In[subscript 0.7]Ga[subscript 0.3]As PHEMTs with f[subscript max] in excess of 1 THz. The devices feature a Pt gate sinking process to effectively thin down the In[subscript ...

  20. Brzozowski's algorithm (co)algebraically F. Bonchi1, M.M. Bonsangue2,3, J.J.M.M. Rutten3,4, A.M. Silva3,4,5

    E-Print Network [OSTI]

    Rutten, Jan

    algebraically, as a function of type X × A X and coal- gebraically, as a function of type X XA. Next, we

  1. Percutaneous needle treatment of liver tumors

    E-Print Network [OSTI]

    mm x 90mm x 260mm · Autoclavable I. Free Space III. Bovine Liver · Precurved concentric nitinol tubes

  2. Inducing pluripotency and immortality in prostate tumor cells : a stem cell model of cancer progression

    E-Print Network [OSTI]

    Fiñones, Rita Roces

    2009-01-01

    5 mM potassium ferrocyanide, 5 mM potassium ferricyanide, 1in 5 mM potassium ferrocyanide, 5 mM potassium ferricyanide,

  3. Evaluation of I-80 Long-Life Corridor Costs

    E-Print Network [OSTI]

    Santero, Nicholas J; Nokes, William; Harvey, John T

    2005-01-01

    Concrete Pipe 450-mm Corrugated Steel Pipe (2.01 mm Thick) 750-mm Corrugated Steel Pipe (2.77 mm Thick) Permeable

  4. Takahiro Matsuda, Takahiko Furuya, Ryutarou Ohbuchi, Lightweight binary voxel shape features for 3D data matching and retrieval, Accepted, Proc. First IEEE Int'l Conf. on Multimedia Big Data (BigMM) 2015, 20-22 April 2015, Beijing, China

    E-Print Network [OSTI]

    Ohbuchi, Ryutarou

    for personalized manufacturing by using 3D printers. Kinect and other RGBD cameras are about to realize 3D geometryTakahiro Matsuda, Takahiko Furuya, Ryutarou Ohbuchi, Lightweight binary voxel shape features for 3D, 20-22 April 2015, Beijing, China 1 Lightweight binary voxel shape features for 3D data matching

  5. Please cite this article in press as: M.M. Rogers, et al., HERO: A smart-phone application for location based emissions estimates, Sustain. Comput.: Inform. Syst. (2014), http://dx.doi.org/10.1016/j.suscom.2014.09.001

    E-Print Network [OSTI]

    Shi, Weisong

    2014-01-01

    on a model that estimates air emission rates of user-selected pollutants based on real-time spatially created that provides consumers with real-time information about local air emissions resulting from- ator is associated with a unique profile of air emissions, based on the type of fuel consumed

  6. Els UK Job: CDI ch09-i047172 16-11-2007 4:15p.m. Page:325 Trim:165240MM Float:Top/Bot TS: Integra, India Fonts: Palatino & Helvetica 9/11 Margins:Top:4PC Gutter:5PC T. W:30PC open recto 1 Color 49 Lines

    E-Print Network [OSTI]

    Oren, Shmuel S.

    markets was not consistent with ERCOT's deregulated wholesale and retail markets. In the economic Perspectives and Divergent Paths PARVIZ ADIB,1 ERIC SCHUBERT,1 AND SHMUEL OREN2 1 Automated Power Exchange, Santa Clara, California, USA and BP North America Gas and Power, Houston, Texas, USA; 2 University

  7. Els UK Job: CDI Ch01-I047172 30-10-2007 9:17a.m. Page:25 Trim:165240MM Float:Top/Bot TS: Integra, India Fonts: Palatino & Helvetica 9/11 Margins:Top:4PC Gutter:5PC T. W:30PC open recto 1 Color 49 Lines

    E-Print Network [OSTI]

    Oren, Shmuel S.

    operations and demand response. Moreover, the optimal extent of vertical integration is ultimately determined

  8. ADVANCED DIGITAL CINEMA CAMERA CAGE 14 E. Jackson St. Suite LL103

    E-Print Network [OSTI]

    Schaefer, Marcus

    ADVANCED DIGITAL CINEMA CAMERA CAGE 14 E. Jackson St. Suite LL103 dcstage, 75mm, 100mm Zeiss CP.2 Cinema Prime Package (EF / Canon Mount) 21mm, 25mm, 35mm

  9. Mfge8 is critical for mammary gland remodeling during involution

    E-Print Network [OSTI]

    2005-01-01

    Rockford, IL) in 5 mM potassium ferrocyanide crystalline, 5mM potassium ferrocyanide trihydrate, and 2 mM magnesium

  10. Anything But Routine: A Selectively Annotated Bibliography of William S. Burroughs v. 1.0.

    E-Print Network [OSTI]

    Schottlaender, Brian E.C.

    2008-01-01

    Extract from The Wild Boys. [M&M]. C307. UFO, No. 1 (June1971). {M&M C308 & 309} ? ?UFO Space Bulletin—?Revolutiontranslation. [M&M] C308. UFO, No. 2 (October 1971). {M&M

  11. ANYTHING BUT ROUTINE: A Selectively Annotated Bibliography of William S. Burroughs v. 2.0

    E-Print Network [OSTI]

    Schottlaender, Brian E.C.

    2010-01-01

    Extract from The Wild Boys. [M&M]. C309. UFO, No. 1 (June1971). {M&M C308 & 309} ?UFO Space Bulletin—?Revolutiontranslation. [M&M] C310. UFO, No. 2 (October 1971). {M&M

  12. Anything But Routine: A Selectively Annotated Bibliography of William S. Burroughs, v. 3.0

    E-Print Network [OSTI]

    Schottlaender, Brian E.C.

    2012-01-01

    Extract from The Wild Boys. [M&M]. C311. UFO, No. 1 (June1971). {M&M C308 & 309} • “UFO Space Bulletin—‘Revolutiontranslation. [M&M] C312. UFO, No. 2 (October 1971). {M&M

  13. Expression analysis of the CLE signaling gene family in Arabidopsis thaliana and functional characterization of CLE8 in seed development

    E-Print Network [OSTI]

    Fiume, Elisa

    2010-01-01

    that 0.5 mM potassium ferrocyanide and 2.5 mM potassiumthat 1mM potassium ferrocyanide and 1mM potassium

  14. Design and Fabrication of a High Aspect Ratio Cable for a High Gradie nt Quadrupole Magnet

    E-Print Network [OSTI]

    Scanlan, R.M.

    2011-01-01

    0 25 mm Illick x 9.5 mm wide polyimide, followed with a .05mm x 9.5 mm wide polyimide film wound with a 2JllOl gap (

  15. A Role for Thrombospondin-1 Deficits in Astrocyte-Mediated Spine and Synaptic Pathology in Down's Syndrome

    E-Print Network [OSTI]

    Garcia, Octavio; Torres, Maria; Helguera, Pablo; Coskun, Pinar; Busciglio, Jorge

    2010-01-01

    M), trolox (100 m M), resveratrol (100 m M), nicotinamide (mM), Trolox (100 m M), resveratrol (100 mM), nicotinamide (mM); trolox (100 m M); resveratrol (Resv, 100 mM); nicotin-

  16. Description The SPCM-AQR is a self-contained module

    E-Print Network [OSTI]

    Saffman, Mark

    : $ 170 mm SPCM-AQR-2X: $ 425 mm · Timing Resolution of 300ps FWHM · User Friendly Applications · LIDAR

  17. TBx18 and the epicardium in cardiac development and regenerative medicine

    E-Print Network [OSTI]

    Martin, Jody Carl

    2008-01-01

    K-Ferricyanide, 50mM K-Ferrocyanide, 200mM MgCl 2 , 100mg/mlK-Ferricyanide, 50mM K-Ferrocyanide, 200mM MgCl 2 , 100mg/mlFerricyanide, 50mM K-Ferrocyanide, 200mM MgCl 2 , 100mg/ml

  18. Application Form Reference Number

    E-Print Network [OSTI]

    Po, Lai-Man

    /yyyy) (/) Title and Description of License/ Certificate/Activity // Date of Award (mm/yyyy) (/) Name Degree/Level Achieved Major Full-time or Part-time Date of Award (mm/yyyy) (/) Period From (mm-time Date of Award (mm/yyyy) (/) Period From (mm/yyyy) (/) To (mm/yyyy) (/) School

  19. Moving Towards a Holistic View of

    E-Print Network [OSTI]

    Gray, Matthew

    /32" (15mm) plywood decking Above grade exterior walls 2" x 6" wood studs @ 16" (400mm) o/c, #15 organic" wood studs @ 24" (600mm) o/c, R13 fiberglass batt insulation, poly vapor barrier, 12mm gypsum board 1, 12mm gypsum board Partition walls 2"x4" wood studs @ 16" (400mm) o/c, 12mm gypsum board two sides 1

  20. Two new orchid bees of the subgenus Euglossella from Peru

    E-Print Network [OSTI]

    Hinojosa-Dí az, Ismael A.; Engel, Michael S.

    2007-01-01

    process; gonostylus thumb-like. Description: d: Structure. Total body length 13 mm; labiomaxillary complex in repose surpassing metasoma by -1 mm (Figs 1-2). Head length 3.31 mm, width 3.15 mm; upper interorbital distance 2.69 mm; lower interorbital... distance 2.38 mm; upper clypeal width 1.27 mm (as measured between dorso­ lateral angles of clypeus); lower clypeal width 2.25 mm (as measured at level of lower lateral parts); clypeal protuberance 0.8 mm (following measurement method of BROOKS, 1 988...

  1. On-Site Wastewater Treatment Systems: Soil Particle Analysis Procedure 

    E-Print Network [OSTI]

    Lesikar, Bruce J.

    2005-08-18

    diameter Fine Fine gravelly 5 to 20 mm diameter Medium Medium gravelly 20 to 75 mm diameter Coarse Coarse gravelly 75 to 250 mm diameter Cobbles Cobbly 250 to 600 mm diameter Stones Stony ?600 mm diameter Boulders Bouldery Flat: 2 to 150 mm long Channers... Channery 150 to 380 mm long Flagstones Flaggy 380 to 600 mm long Stones Stony ?600 mm long Boulders Bouldery 1 The roundness of fragments may be indicated as angular (has strongly developed faces with sharp edges), irregular (has prominent flat faces...

  2. Slide 1

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    the end of delithiation Linda Y. Lim et. al., submitted to Chem. Mater. BL 11-3: Watching Batteries In-operando 2 mm 2 mm 2 mm 2 mm 2 mm 0.4 mms 1.6 mms 2.8 mms 4 mms 8 mms...

  3. UNIVERSITY OF EAST ANGLIA School of Computing Sciences

    E-Print Network [OSTI]

    Janacek, Gareth

    manipulation and exploration. 4. Reporting of problem and solution. As always, credit is given for a persuasive techniques to examine the data set and report your findings. 80% The columns are · FL frontal lobe size (mm) · RW rear width (mm) · CL carapace length (mm) · CW carapace width (mm) · BD body depth (mm) GJJ/2c22p2

  4. Recovery of Sugars from Ionic Liquid Biomass Liquor by Solvent Extraction

    E-Print Network [OSTI]

    Brennan, Timothy C.; Datta, Supratim; Blanch, Harvey W.; Simmons, Blake A.; Holmes, Bradley M.

    2010-01-01

    in the IL/ water phase before extraction was 10 mM and atin the IL/ water phase before extraction was 10 mM and atin the IL/ water phase before extraction was 10 mM and at

  5. Management Overview

    Energy Savers [EERE]

    so only a half cross-section of the set-up is shown The test tube is 12mmOD with 1 mm thick walls and 50 mm long 1000 psi internal applied pressure 950C Welds...

  6. Multisensory and sensorimotor representations for action in human posterior parietal cortex investigated with functional MRI

    E-Print Network [OSTI]

    Filimon, Flavia

    2008-01-01

    36 Table 2. Average MNI-space coordinates (in mm) for36 Table 3. Average MNI-space coordinates (in mm) for130 Table 2. Average MNI-space coordinates (mm) for peak

  7. Millimeter-Wave Circuits for 60GHz and Beyond

    E-Print Network [OSTI]

    Afshar, Bagher

    2010-01-01

    Device Modeling for mm-Wave Design . . . . . . . . . .Devices for mm-Wave Design . . . . . . . . . . . . . .9.2 Previous Work on mm-Wave Power Ampli?ers in SiGe

  8. Correlation of mechanical viscoelastic properties to microstructure of equine cortical bone tissue 

    E-Print Network [OSTI]

    Ayers, Andrew Kerr

    1995-01-01

    were taken from equine third metacarpal bones and machined into rectangular slabs approximately 46 mm long, 10 mm wide, and 2 mm thick. After initial testing to determine the linear viscoelastic region of equine compact bone, the specimens were tested...

  9. Lean-MeanLean-Mean Skating MachineSkating Machine

    E-Print Network [OSTI]

    Levi, Anthony F. J.

    , Bamboo Trucks: Randal 180mm Wheels: Orangutang Freerides (70mm, 86a) Bushings: Venom Bushings (80a) #12: Sector 9 Slalom Wheels (70mm, 86a) Bushings: Venom Bushings (80a) #12;Experimental Controls

  10. New Rotary Engine Designs by Deviation Function Method

    E-Print Network [OSTI]

    Warren, Sarah

    2012-01-01

    of apex seals in a Wankel engine, R = 105 mm. . . . . . . .of 2 mm apex seals in a Wankel engine, R = 105 mm. . .9] D. E. Cole. The wankel engine. Scientific American, 227:

  11. New Rotary Engine Designs by Deviation Function Method

    E-Print Network [OSTI]

    Warren, Sarah

    2012-01-01

    of apex seals in a Wankel engine, R = 105 mm. . . . . . . .2 mm apex seals in a Wankel engine, R = 105 mm. . . Radius9] D. E. Cole. The wankel engine. Scientific American, 227:

  12. Synthesis, Postmodification, Metalation, and Gas Adsorption in Chemically Stable Metal Organic Frameworks and Zeolitic Imidazolate Frameworks.

    E-Print Network [OSTI]

    Morris, William

    2012-01-01

    4 mm (outside diameter) zirconia rotors. The magic angle was4 mm (outside diameter) zirconia rotors. The magic angle was4 mm (outside diameter) zirconia rotors. The magic angle was

  13. Fuzzy-probabilistic calculations of evapotranspiration

    E-Print Network [OSTI]

    Faybishenko, B.

    2013-01-01

    potential evapotranspiration (mm/day); R s = daily global (total) solarpotential evapotranspiration (mm day -1 ); R s = daily global (total) solarpotential evapotranspiration (mm day -1 ); R s = monthly mean of daily global (total) solar

  14. Acute dosing of latrepirdine (DimebonTM), a possible Alzheimer therapeutic, elevates extracellular amyloid-beta levels in vitro and in vivo

    E-Print Network [OSTI]

    Steele, John W.; Kim, Soong Ho; Cirrito, John R.; Verges, Deborah K.; Restivo, Jessica L.; Westaway, David; Fraser, Paul; St George Hyslop, Peter; Sano, Mary; Bezprozvanny, Ilya; Ehrlich, Michelle E.; Holtzman, David M.; Gandy, Sam

    2009-12-17

    was collected following 6 hours of treatment, cells were washed 1× with ice cold PBS, and cells were lysed and collected in 1× lysis buffer [20 mM Tris, 137 mM NaCl, 1 mM EDTA, 1 mM pepstatin, 1 mM PMSF, 5 mM ZnCl2, 1% Triton X-100, EDTA-free mini- complete...

  15. The seventeenth International Symposium on Transport Phenomena, 4-8 September, 2006, Toyama, JAPAN

    E-Print Network [OSTI]

    Kasagi, Nobuhide

    -plated polyimide film of 9 mm in length and 3 mm in width. The thicknesses of polyimide and copper layers are 25 µm

  16. Microsoft PowerPoint - KTH_pres - Leif Kari.pptx

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    sources fiber contact wire 100 mm 1 mm Nanostruct. Physics (9 p) Quantum circuits, spintronics, nano- bio surfaces, AFM Antibunching Quantum Electr.Opt. (8 p) Quantum...

  17. Insertion Devices

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    Vacuum Chamber The current ID vacuum chamber has a internal vertical aperture of 8 mm allowing for minimum undulator gap of 11 mm The current ID vacuum chamber...

  18. The role of vinculin in cardiac mechanotransduction

    E-Print Network [OSTI]

    2010-01-01

    periscope or penicillin-streptomycin= 300mm), mirror (M), periscope (PS), shutter (S), and half= 300mm), mirror (M), periscope (PS), shutter (S), and half

  19. Sandia National Laboratories: Research: Facilities: Technology...

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    for counterterrorism hydrocode validation Available Launchers 100 mm compressed gas gun (velocities to 1 kms) 100 mm compressed light gas gun for oblique impacts (velocities...

  20. Formulation Sheet JBScreen HTS I

    E-Print Network [OSTI]

    Hill, Chris

    .5 200 mM Lithium Sulfate A 5 30 % w/v PEG 400 None 100 mM Sodium Acetate 4.6 100 mM Calcium Chloride A 6 2 Buffer pH Additive A 1 15 % w/v PEG 400 None 100 mM Sodium Acetate 4.6 100 mM Calcium Chloride A 2 None 100 mM Sodium Acetate 4.6 100 mM Magnesium Chloride A 4 25 % w/v PEG 400 None 100 mM Tris-HCl 8

  1. Use of Sm-123 + Sm-211 Mixed-powder Buffers to Assist the Growth of SmBCO and ZrO2-doped SmBCO Single Grain, Bulk Superconductors

    E-Print Network [OSTI]

    Zhao, Wen; Shi, Yunhua; Dennis, Anthony R.; Cardwell, David A.

    2014-12-18

    motorized pestle and mortar was used to mix thoroughly powders of composition (75 wt% Sm-123 + 25 wt% Sm-211) + 2 wt% BaO2 + 1 wt% CeO2, prior to being pressed uniaxially under a pressure of 1.5 tons into a green pre-form (pellet-like) with diameters... of 20 mm and 25 mm and thicknesses of 9 mm and 12.5 mm (each pellet shrinks to about 80 % of its original size after TSMG, corresponding to as processed dimensions of 16 mm and 20 mm diameter and 7 mm and 10 mm thickness). Doped green pellets were...

  2. High power density supercapacitors using locally aligned carbon nanotube electrodes

    E-Print Network [OSTI]

    Du, C S; Yeh, J; Pan, Ning

    2005-01-01

    carbon nanotubes in 1 ml of DMF) on two 12 mm × 12 mm nickelnanotubes as electrodes. An [7, 15] obtained high power density with polished nickel

  3. SUPPLEMENTARY INFORMATION 1www.nature.com/nature

    E-Print Network [OSTI]

    Schnitzer, Mark

    /kg ketamine and 5mg/kg xylazine). The top of the animal's head was shaved, cleaned with 70 % ethanol into the motor cortex (2.0 mm AP; 1.42 mm ML, two injections at -1.25 mm and -1.75 mm DV) of 5- 10-week

  4. Foldable Printed Circuit Boards on Paper Substrates By Adam C. Siegel, Scott T. Phillips, Michael D. Dickey, Nanshu Lu,

    E-Print Network [OSTI]

    Prentiss, Mara

    of polyimide (25 mm thick), ii) a layer of adhesive (25 mm thick), iii) a layer of copper (36 mm thick), iv) a second layer of adhesive (25 mm thick), and v) a cover layer of polyimide. Although this method PCBs, offers a set of properties that are completely different from the properties of polyimide

  5. The Evolution of Tooling, Technical and Quality Control for Accelerator Dipole Magnet Applications

    E-Print Network [OSTI]

    Scanlan, R.M.

    2011-01-01

    mimimum specification value. "Inis _presented a significanttolerance, or + .003 mm. 'Inis requirementcan be met, but it

  6. MJG:Peer Review, 5/00 1 M. J. Gouge

    E-Print Network [OSTI]

    -screw extruder (2-mm hydrogen extrusions). · ORNL is exploring (concept design) double-screw and gear

  7. Functions of Leucine Rich Repeat Receptor-Like Kinases (LRR-RLKs) in Arabidopsis Sexual Reproduction

    E-Print Network [OSTI]

    Khamsuk, Ornusa

    2011-01-01

    pH 7.0, 0.5 mM potassium ferrocyanide, 0.5 mM potassiumpH 7.0, 0.5 mM potassium ferrocyanide, 0.5 mM potassium

  8. Y.M. Zhang, A.T. Male, M. Jiang, S.Zhang University of Kentucky

    E-Print Network [OSTI]

    Zhang, YuMing

    Compensation Through Thickness #12;Energy Distribution: Regular Plasma Arc Plasma arc Plasma arc Efflux plasmaXF Plasma current 150 A 200 A 180 A Double-sided arc current 100 A 110 A 110 A Welding speed 90 mm cfh 35 cfh 35 cfh Plasma orifice diameter 2 mm 2 mm 2 mm Double-sided arc shielding gas flow rate 55

  9. DNS of complex fuel combustion with detailed chemistry: physical insight and mean reaction rate modelling

    E-Print Network [OSTI]

    Nikolaou, Z. M.; Swaminathan, N.

    2015-01-01

    The computational domain has Lx = 14 mm and Ly = Lz = 7 mm with corresponding number of grid points Nx = 768 and Ny = Nz = 384 for case A. These values for case B are Lx = 21 mm, Ly = Lz = 7 mm, Nx = 1632 10 and Ny = Nz = 544. The numerical resolution is dictated...

  10. Probing the ArcA regulon under aerobic/ROS conditions in Salmonella enterica serovar Typhimurium

    E-Print Network [OSTI]

    2013-01-01

    cells Glycolysis/gluconeogenesis Biosynthesis of siderophoreMM: Glycolysis, gluconeogenesis, and the pentose phosphate

  11. On the Randomness of the Editing Generator Enjian Bai and Guozhen Xiao

    E-Print Network [OSTI]

    International Association for Cryptologic Research (IACR)

    that is called the editing generator (and referred to as EG) is introduced [7]. The EG is a sequence generator. For four special cases, (m-sequence, mm-sequence)-EG, (mm-sequence, mm-sequence)- EG, (m-sequence, m-sequence)-EG, and (mm-sequence, m-sequence)-EG, the randomness of the edited sequence is discussed in detail

  12. Dynamically tokamakreactor

    E-Print Network [OSTI]

    Zakharov, Leonid E.

    plasma facing lithium streams driven by magnetic propulsion, b)' 1 mm thick patchy separation guide wall

  13. JBS Crystallization Freshman Kit Scholar Cat.-No: CSK-102 Get a head start crystallizing your protein

    E-Print Network [OSTI]

    Lebendiker, Mario

    mM Lithium Sulfate D 4 30 % w/v PEG 4000 None 100 mM Tris-HCl 8.5 200 mM Sodium Acetate D 5 30 % w Number Precipitant 1 Precipitant 2 Buffer pH Additive A 1 15 % w/v PEG 400 None 100 mM Sodium Acetate 4.5 200 mM Sodium Citrate A 5 25 % w/v PEG 400 None 100 mM Sodium Acetate 4.6 100 mM Magnesium Chloride

  14. Dr. Campbell's Bio111 Exam #1 Fall 2001 Fall 2001 Biology 111 Exam #1 -Cellular Communications

    E-Print Network [OSTI]

    Campbell, A. Malcolm

    ): Write out the full pledge and sign: How long did this exam take you to complete (excluding typing)? #12L solution that is 1.44 mM NADP+ , 50 mM isocitrate and 7% v/v IDH if your stock solutions are 28.8 mM NADP+ , 500 mM isocistrate and 100 mM IDH (to be considered 100% IDH stock solution). 7 pts. 2) In the graph

  15. Revision of the orchid bee subgenus Euglossella (Hymenoptera, Apidae), Part I, The decorata species group

    E-Print Network [OSTI]

    Hinojosa-Dí az, Ismael A.; Engel, Michael S.

    2011-10-26

    ) (Fig. 15). Description. ?: Structure. Total body length 12.44 mm; labiomaxillary complex in repose reaching posterior tip of metasoma (estimate) (Fig. 8). Head length 2.85 mm, width 5.11 mm; upper interorbital distance 2.44 mm; lower interorbital... angles of clypeus); lower clypeal width 2.09 mm (2.02–2.15; n=5) (as measured at level of lower lateral parts); clypeal protuberance 0.67 mm (0.52–0.81; n=5) [following measurement method of Brooks(1988)]; clypeal ridges, labral ridges Ismael A...

  16. The attempted synthesis of arginine adenylate and the sterochemical determination of the MgATP complex of argininosuccinate 

    E-Print Network [OSTI]

    Shull, Timothy Barton

    1987-01-01

    -piperazineethanesulfonic acid (HEPES), inorganic pyrophospha- tase (PPase), lactate dehydrogenase (LDH), 2-(N-morpholino) ethanesul- fonic acid (MES), myokinase (adenylate kinase), pyruvate kinase, and tris(hydroxymethyl)aminomethane (TRIS) were obtained from Sigma. DE... contained 10 mM ADPPS, 15 mM PEP, 12 mM magnesium acetate, 0. 25 mM EDTA, 100 mM HEPES, pH 8. 0, 100 mM KCI, and 0. 30 mg pyruvare kinase in a volume of 5. 0 mL. The reaction was incubated at 30 '0 for 3 hours. The 30 reaction was followed by HPLC...

  17. SU-E-J-171: Surface Imaging Based Intrafraction Motion Assessments for Whole Brain Radiotherapy

    SciTech Connect (OSTI)

    Wiant, D; Vanderstraeten, C; Maurer, J; Pursley, J; Terrell, J; Sintay, B

    2014-06-01

    Purpose: To quantify and characterize intrafraction motion for whole brain radiotherapy treatments in open face masks using 3D surface imaging. Methods: Fifteen whole brain patients were monitored with 3D surface imaging over a total of 202 monitoring sessions. Mean translations and rotations were calculated over each minute, each session, and over all sessions combined. The percentage of each session that the root mean square (RMS) of the linear translations were outside of 2 mm, 3 mm, 4 mm, and 5 mm were determined for each patient. Correlations between mean translations per minute and time and between standard deviation per minute and time were evaluated using Pearson's r value. Results: The mean RMS translation averaged over all patients was 1.45 mm +/? 1.52 mm. The patients spent an average of 18%, 10%, 6%, and 3% of the monitoring time outside of 2 mm, 3 mm, 4 mm, and 5 mm RMS tolerances, respectively. The RMS values averaged over all patients were 1.31 mm +/? 0.98 mm, 1.52 +/- 1.04, and 1.30 mm +/? 0.71 mm over the 1th, 5th, and 10th minutes of monitoring, respectively. Neither, the RMS values (p = 0.15) or the standard deviations of the RMS values (p = 0.16) showed significant correlations with time. Conclusion: The patients were positioned within 2 mm of isocenter, which was the initial set-up tolerance, for the majority of their treatments. The average position changed by < 0.3 mm over 10 minutes of monitoring. Short term movements, reflected by the standard deviations, where on the order of 1 mm. This immobilization system provides adequate immobilization over a course of treatment for whole brain radiotherapy. This system may also be suitable for head and neck or stereotactic radiosurgery treatments as well.

  18. Sandia Energy - EC Publications

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    AL Lentine Micro-optical 5mm lenses in 50mm sub-arrays illuminate arrays of photovoltaic cells with 49X concentration. Fine tracking over 100 FOV in sub-array...

  19. Modulating Protein Activity through Polymer Conjugation

    E-Print Network [OSTI]

    Decker, Caitlin Gayle

    2015-01-01

    the   polymer  backbone,  but  100  mM  carbonate  /  carbonate   /   bicarbonate  (pH  10)  buffer  partially   degraded  the  polymer  polymer  2  in   either  D-­PBS  or  100  mM  carbonate  /  

  20. InGaAsP/InP intrastep quantum wells for enhanced solar energy conversion

    E-Print Network [OSTI]

    Chen, Winnie Victoria

    2012-01-01

    photon was able to pick up one solar photon converted tothe efficiency of a solar cell with one bandgap, CH Henry’sArray of four solar cells on one 10mm by 10mm substrate

  1. Periodic and Disordered Structures in a Modulated Gas-Driven Granular Layer I. S. Aranson,1

    E-Print Network [OSTI]

    Tsimring, Lev S.

    when the drag force exerted by the fluid on the granulate exceeds gravity. A uniform fluidization to 12 mm. We typically used 0.15 mm diameter bronze spheres or 0.2

  2. Microfluidic advantage : novel techniques for protein folding and oxygen control in cell cultures

    E-Print Network [OSTI]

    Polinkovsky, Mark E.; Polinkovsky, Mark E.

    2012-01-01

    have 20 mm long segments of polyimide-coated fused-silicaA segment of 18-gauge polyimide tubing is inserted into thehas a 15 mm long 21-gauge polyimide capillary inserted into

  3. Terrestrial water mass load changes from Gravity Recovery and Climate Experiment (GRACE)

    E-Print Network [OSTI]

    Seo, K.-W.; Wilson, C. R; Famiglietti, J. S; Chen, J. L; Rodell, M.

    2006-01-01

    3d is the dynamic filter water storage map using GRACE SHfrom the four basin filters in mm water thickness. Noisefrom the four basin filters in mm water thickness. Error

  4. Photochemical Disinfection of Escherichia coli in the Presence of Natural Aquatic Sensitizers: Influence of Solution Chemistry and Extracellular Polymeric Substances

    E-Print Network [OSTI]

    Gong, Amy Shin Hwei

    2011-01-01

    three surfaces, for cells with full and partial EPS at 10mM KCl, zeta potential of full EPS cells was observed to befound with full and partial EPS coated cells in 1 and 10 mM

  5. Tropical Daytime Lower D-region Dependence on Sunspot Number Neil R. Thomson and Craig J. Rodger

    E-Print Network [OSTI]

    Otago, University of

    and then on to Kauai, Hawaii, ~10.6 Mm from NWC. Observations24 from the 8.1-Mm path NPM (21.4 kHz, Hawaii) to Dunedin

  6. Project Profile: Encapsulated Phase Change Material in Thermal...

    Office of Energy Efficiency and Renewable Energy (EERE) Indexed Site

    way to produce small 10 mm to 15 mm capsules containing phase change material (PCM salt) in a suitable shell material. Large numbers of these PCM capsules provide high-heat...

  7. LIMITATIONS ON THE RESOLUTION OF YAG:CE BEAM PROFILE MONITOR...

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    performance to other diagnostics. 2 Experimental Set-up And Initial Results An aluminum-base target was constructed with the two YAG:Ce crystals (0.50 mm and 0.25 mm thick...

  8. Herpetological Review 42(2), 2011 291291nAtuRAl hiStORy nOteS 291

    E-Print Network [OSTI]

    Langford, Gabriel

    dipsadid snake that is widely distributed in northern South America. This species inhabits ponds, streams, an adult female H. angulatus (SVL = 490 mm; tail length = 215 mm) was collected near the Un- ini river

  9. A reproducible and low-cost piezoelectric droplet generator

    E-Print Network [OSTI]

    Liu, Tanya

    2014-01-01

    This thesis presents the design for a piezoelectric droplet generator capable of producing highly repeatable droplets ranging from 0.60 mm to 1.60 mm in diameter. The generator is low cost, simple to fabricate, and easily ...

  10. CX-001004: Categorical Exclusion Determination | Department of...

    Energy Savers [EERE]

    items), and supervision required to perform the work associated with West Hackberry (WH)-MM-589 and WH-MM-730. DOCUMENT(S) AVAILABLE FOR DOWNLOAD CX-001004.pdf More Documents &...

  11. Modulation of intermolecular interactions in single- molecule magnets

    E-Print Network [OSTI]

    Heroux, Katie Jeanne

    2010-01-01

    76 2.3.5. Electrochemistry…………………………………………………………82 2.4.82 Figure 2.18. Electrochemistry of 5 mM solution of “Mn 383 Figure 2.19. Electrochemistry of 3 (top, 1 mM solution in

  12. Supplementary Figure 5 Analytical ultra-centrifugation indicated that Rad54 is monomeric in solution.

    E-Print Network [OSTI]

    Kowalczykowski, Stephen C.

    ). Addition of 5mM AMP-PNP and 10mM MgCl2 gave a MWobs ~ 98 +/- 2.7kDa (B). Addition of a double stranded 21

  13. Using Nanotechnology in Agriculture Kent Pinkerton, Ph.D.

    E-Print Network [OSTI]

    Leistikow, Bruce N.

    Laser only 17 mm 20 mm Untreated No Residual MWCN T + Laser #12;Aerogels (Frozen Smoke) for Increased Insulation and Energy Storage Image Source: NASA Jet Propulsion Lab (http://stardust.jpl.nasa.gov/photo/aerogel

  14. Molecular scale biocomputing : an enzyme logic approach

    E-Print Network [OSTI]

    Windmiller, Joshua Ray; Windmiller, Joshua Ray

    2012-01-01

    i) and 10mM potassium ferrocyanide solution (ii). To examineii) 10mM potassium ferrocyanide. First five initial scanningalso occurred in the ferrocyanide solution (ii), where the

  15. Passive millimeter-wave retrieval of global precipitation utilizing satellites and a numerical weather prediction model

    E-Print Network [OSTI]

    Surussavadee, Chinnawat

    2007-01-01

    This thesis develops and validates the MM5/TBSCAT/F([lambda]) model, composed of a mesoscale numerical weather prediction (NWP) model (MM5), a two-stream radiative transfer model (TBSCAT), and electromagnetic models for ...

  16. The Kinetochore Protein Mif2p is Targeted by Cdk1p and Development of a Selection for Regulators of Centromere/Kinetochore Structure/Function

    E-Print Network [OSTI]

    Wallace, Isha

    2010-01-01

    to a standard yeast lithium acetate protocol. Briefly, ~1µga solution of 100 mM lithium acetate, 10 mM tris, pH 8.0, 1

  17. phys. stat. sol. (c) 4, No. 3, 838842 (2007) / DOI 10.1002/pssc.200673847 2007 WILEY-VCH Verlag GmbH & Co. KGaA, Weinheim

    E-Print Network [OSTI]

    Johnson, Peter D.

    2007-01-01

    , 9700 South Cass Avenue, Argonne, IL 60439, USA 3 Condensed Matter Physics & Materials Science] ~3.5 mm square and nominally 1.5 mm thick were cut and polished with a wedged back surface to avoid

  18. LIFE

    E-Print Network [OSTI]

    sured 4 years previously, and so on, and this column constitutes an ultimate mortality ... 1,4,3 in the ultimate column. The complete ... gig: mm] = 1mm = 940,108.

  19. Microsoft Word - PAC99 Final Version.doc

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    of the cathode. A 1 mm accelerating gap was used, with a potential of 1 MV on the cathode. The emitting spot had a radius of .25 mm and the initial transverse and longitudinal...

  20. Encoding externally and internally accredited value in prefrontal cortex

    E-Print Network [OSTI]

    Luk, Chung-Hay

    2011-01-01

    i.e. , apple juice or quinine. Again, PFcs had more rewarddilution, Safeway), and quinine (1.1 mM, Sigma-Aldrich). Fordilution), apple juice, and quinine (3.3 mM). We note that

  1. SU-E-T-183: Feasibility of Extreme Dose Escalation for Glioblastoma...

    Office of Scientific and Technical Information (OSTI)

    Original VMAT plans were created with 2 to 4 coplanar or non-coplanar arcs using 3 mm hi-res MLC. The 4 optimization, using 5 mm MLC, selected and inverse optimized 30 beams...

  2. Coupled Physics Inverse Problems: EIT meets MRI

    E-Print Network [OSTI]

    2013-11-14

    Nov 14, 2014 ... about 1 mm (New MRI, INUMAC (Imaging of Neuro disease Using high-field MR And Contrastophores) 11.75-Tesla resolves up to. 0.1mm).

  3. Organic synthesis as an effective approach to chemical, pharmaceutical, and biosynthetic investigations of natural products

    E-Print Network [OSTI]

    Suyama, Takashi L.

    2009-01-01

    mm Synergi 4? Hydro- RP 80A column, MeCN/H 2 O gradient) tousing a Synergi 4? Hydro-RP 80A (250 x 10 mm) column (1.2

  4. A simple method for enzymatic synthesis of unlabeled and radiolabeled Hydroxycinnamate-CoA

    E-Print Network [OSTI]

    Rautergarten, Carsten

    2012-01-01

    column (Synergy 4u Fusion-RP 80A 250× 2.0 mm, Phenomenex,column (Synergy 4u Fusion-RP 80A 250× 10.0 mm, Phenomenex)

  5. A Simple Method for Enzymatic Synthesis of Unlabeled and Radiolabeled Hydroxycinnamate-CoA

    E-Print Network [OSTI]

    Rautengarten, Carsten; Baidoo, Edward; Keasling, Jay D.; Scheller, Henrik Vibe

    2010-01-01

    column (Synergy 4u Fusion-RP 80A 250× 2.0 mm, Phenomenex,column (Synergy 4u Fusion-RP 80A 250× 10.0 mm, Phenomenex)

  6. long-term electricity harvesting in open systems such as sedimentary environments.

    E-Print Network [OSTI]

    Helsinki, University of

    . 13. A dual-chambered fuel cell was constructed using 54-mm OD (outside diameter) glass tubing and a 22-mm OD pinch clamp assembly. Electrodes used in dual-chamber fuel cells had a surface area of 25

  7. Carbon Emissions from Smouldering Peat in Shallow and Strong Fronts 

    E-Print Network [OSTI]

    Rein, Guillermo; Cohen, Simon; Simeoni, Albert

    2009-01-01

    A series of experiments of shallow and strong smouldering fronts in boreal peat have been conducted under laboratory conditions to study the CO and CO2 emissions. Peat samples of 100 mm by 100 mm in cross section and 50 ...

  8. Magnet Cable Manufacturing

    E-Print Network [OSTI]

    Royet, J.M.

    2011-01-01

    mid thickness Cable width Keystone angle 1.458 mm 9.296 mm (diameter Mid Thickness Width Keystone angle ±2.5Ilm ±6. 35least one roller ground to the keystone angle. However, such

  9. Barriers and Facilitators in the Recruitment and Retention of Peruvian Female Sex Workers in a Randomized HPV Vaccine Trial

    E-Print Network [OSTI]

    2013-01-01

    7747. 3. Brown B, Blas MM, Cabral A, Carcamo C, Gravitt P,Janni Kinsler 2 , Alejandra Cabral 3 , Magaly M Blas 4 ,N, Brown B, Kinsler J, Cabral A, Blas MM, et al. (2013)

  10. Geophysical Fluid Dynamics Laboratory Review June 30 -July 2, 2009

    E-Print Network [OSTI]

    temperature (K) Precipitation (mm day1) AERO GAS BOTH SUM AERO GAS BOTH SUM Ming and Ramaswamy (2009

  11. DAY 1 Monday, March 11, 2013 Place Lobby, 1F

    E-Print Network [OSTI]

    Hung, Shih-Hao

    Collaborative Approach in 450mm Transition, per an SME Perspective Mr. Alain Jarre Chairman and CEO, RECIF

  12. Pressure Losses in 12”, 15” and 16” Non-Metallic Flexible Ducts with Compression and Sag (RP-1333) 

    E-Print Network [OSTI]

    Culp, C.H.; Cantrill, D.

    2009-01-01

    is based on findings resulting from ASHRAE Research Project RP-1333. ABSTRACT A study was conducted to measure air pressure loss in non- metallic flexible ducts and included 12” (305 mm), 14” (356 mm) and 16” (406 mm) diameter ducts on a flat surface... and also positioned over joists on 24” (610 mm) centers. For this study, flexible duct compression configurations were fully stretched and 4%, 15%, 30% and 45% compressed. Measure- ments were performed at each compression. All tests were performed...

  13. Original Research Imaging Inflammation: Direct Visualization of

    E-Print Network [OSTI]

    (CIVM) using a 9.4-Tesla, 89-mm bore, superconducting magnet with actively shielded gradients capable

  14. D e s c r i p c i n -O b s e r v a c i o n e s taxonmicas

    E-Print Network [OSTI]

    Murcia, Universidad de

    1,30 a 1,72 mm de longitud. Cuerpo ovalado, de coloración pardo oscura, con leves reflejos metálicos

  15. D e s c r i p c i n -O b s e r v a c i o n e s taxonmicas

    E-Print Network [OSTI]

    Murcia, Universidad de

    . 1,4 mm de longitud) de color marrón con reflejos metálicos en cabeza y pronoto, siendo las patas y

  16. ABSTRACT: RANZI R., GROSSI G., GITTI A. & TASCHNER S., Energy and mass balance of the Mandrone glacier (Adamello, Central Alps). (IT

    E-Print Network [OSTI]

    mm for the 2002/03 year. KEY WORDS: Glacier retreat, Mass balance, Energy balance, Man- drone Glacier

  17. 0044-5231/03/242/02-107 $ 15.00/0 Review of Biogeography, Host Range and Evolution

    E-Print Network [OSTI]

    Lehmann, Gerlind

    phonotactic accuracy, even in darkness; Ormia ochracea landed at a mean distance of 82 mm Zool. Anz. 242 (2003

  18. J Low Temp Phys (2015) 179:914 DOI 10.1007/s10909-014-1240-3

    E-Print Network [OSTI]

    Majós, Antonio Badía

    2015-01-01

    J Low Temp Phys (2015) 179:9­14 DOI 10.1007/s10909-014-1240-3 In Plane Vortex Dynamic Anisotropy with the direction in which the dissipation due to vortex movement is minimum, evidencing the existence of pinning with a platelet shape (typical dimensions: 0.7mm2 × 0.02mm) and others as tubes (3.6 × 10-3 mm2 × 0.2mm). Figure 1

  19. Full lineup serves wide variety of processing needs DAD3220, 3230 or 3430 is a one-axis dicing saw for 6-inch (6-inch square)

    E-Print Network [OSTI]

    for ø6-inch (6-inch square) workpieces. DAD3220, just 500 mm wide, helps conserve valuable cleanroom

  20. Three-dimensional gas temperature measurements in atmospheric pressure microdischarges using Raman scattering

    E-Print Network [OSTI]

    Economou, Demetre J.

    and guided into a periscope, which consisted of a Brewster's angle window, a right angle prism, and a 3 mm

  1. REFINING THE SONIC FLASHLIGHT FOR INTERVENTIONAL PROCEDURES

    E-Print Network [OSTI]

    Stetten, George

    /or color display. For the latest handheld SF, a 54.8mm (diagonal) organic light emitting diode (OLED

  2. Practical Vessel Imaging by Computed Tomography in Live Transgenic Mouse Models for Human Tumors

    E-Print Network [OSTI]

    Capecchi, Mario R.

    delivered by a generic fish tank pump. Volumetric CT of anesthetized mice was per- formed at 93 mm3 voxel

  3. 8. Gutsch, A., Kramer, M., Michael, G., Muhlenweg, H., Pridohl, M., Zimmermann, G.: Gas-phase production of

    E-Print Network [OSTI]

    Nelson, Celeste M.

    , which, when disrupted, lead to aberrant tissue function and disease. At the mesoscale (100­1,000 mm

  4. Impact of Virtual Memory Managers on Performance of J2EE Applications

    E-Print Network [OSTI]

    Murphy, Liam

    : ­ Debian 2.4; ­ Debian 2.6; ­ SUSE; ­ Fedora Core; ­ Alan Cox (-ac); ­ Andrew Morton (-mm); ­ Con Kolivas

  5. which are known to control aspects of plant development. The AG MADS-box gene has a critical function in plant sexual reproduc-

    E-Print Network [OSTI]

    von Andrian, Ulrich H.

    that the concentrations of potassium ferrocyanide and potassium ferricyanide were 5 mM. Plant materials The stk-1 allele

  6. Assessing Exposures to Particulate Matter and Manganese in Welding Fumes

    E-Print Network [OSTI]

    LIU, SA

    2010-01-01

    limit PM: particulate matter PTFE: polytetrafluoroethylenepolytetrafluoroethylene (PTFE) with polymethylpentenethrough the OPC and a 47 mm PTFE filter (Grimm Technologies,

  7. Lesson Summary In this lesson, students will build an open spectrograph to

    E-Print Network [OSTI]

    Mojzsis, Stephen J.

    ") rectangular of 5mm (3/16") thick foam core board · 2-Styrofoam cups · Holographic diffraction grating (1000

  8. The Centers for Disease Control and Prevention's Vessel Sanitation Program is proud to bring to you the following

    E-Print Network [OSTI]

    (254 mm) · Highest form of protection ­ sewage #12;Air gap alternatives Barometric Loop Or Anti-siphon

  9. ANS complex of St John’s wort PR-10 protein with 28 copies in the asymmetric unit: a fiendish combination of pseudosymmetry with tetartohedral twinning

    E-Print Network [OSTI]

    Sliwiak, Joanna; Dauter, Zbigniew; Kowiel, Marcin; McCoy, Airlie J.; Read, Randy J.; Jaskolski, Mariusz

    2015-04-25

    . The pellet was resuspended in lysis buffer [500 mM NaCl, 20 mM Tris–HCl pH 8.0, 20 mM imidazole, 3 mM ?-mercaptoethanol, 100 mg ml?1 chicken egg-white lysozyme (Sigma–Aldrich)] and sonicated. The lysate was centrifuged at 18 000g for 15 min at 277 K...

  10. www.sciencemag.org/cgi/content/full/315/5812/620/DC1 Supporting Online Material for

    E-Print Network [OSTI]

    Lakes, Roderic

    , with diameters of 2.6 mm and 3 cm long, using a wire electron discharge milling machine (EDM). Specimens

  11. Practical realization of massively parallel fiberfree-space optical interconnects

    E-Print Network [OSTI]

    Jahns, Jürgen

    on a computer-controlled milling machine. Channel densities are of the order of 100 mm2 between optoelectronic

  12. Machine Design -2 Consider a machined bar made of cold-drawn 1045 steel shown below. A notch with radius

    E-Print Network [OSTI]

    Battaglia, Francine

    dx dx = = = - Area moment of inertia (Solid rectangular area) 3 12 bh I = Normal stress My I b uta aSk = Surface Finish Factor a (Sut, MPa) Exponent b Ground 1.25 -0.085 Machined/Cold-Drawn 4.51.79mm 51mm 1.51 51mm 254mm e e e b e e d d d k d d - - - = =

  13. ORIGINAL PAPER P. R. Territo J. Altimiras

    E-Print Network [OSTI]

    Altimiras, Jordi

    - metamorphic climax). Surface area [8.5 mm2 at stages Nieuwkoop-Faber (NF) 33±34 to 70.2 mm2 at stages NF 50±51 (hemoglobin poisoning with carbon monoxide), whole animal surface area and volume were measured and bulk] and volume (1.8 mm3 at stages NF 33±34 to 35.7 mm3 at stages NF 50±51) measured from volu- metric analysis

  14. Identification and design of small molecules that associate with aggregated Alzheimer's-related beta-amyloid peptides

    E-Print Network [OSTI]

    Bautista, Mahealani Roberts

    2009-01-01

    Naringenin Quercetin Resveratrol Rutin Scyllo-inositolµM 10mM Concentration of Resveratrol OH HO OH Inhibition (%)

  15. Analysis of Solar Passive Techniques and Natural Ventilation Concepts in a Residential Building Including CFD Simulation 

    E-Print Network [OSTI]

    Quince, N.; Ordonez, A.; Bruno, J. C.; Coronas, A.

    2010-01-01

    are double glazed (10mm + 8mm air + 10mm), with aluminium frame and cold bridge breaking. All apartments are designed to allow cross ventilation. The project of the building (Pastor and Toral 2006) plans two basic natural ventilation mechanisms: a stack...

  16. 10mg Acidic v5.4 Refold Master

    E-Print Network [OSTI]

    Lebendiker, Mario

    .4 Page 1 Table of Contents Introduction .................................. 2 ­ 3 Kit Contents #12;10mg Acidic v5.4 Page 4 Kit Contents ­ Ready for Use A ­ Denaturation buffer (4.9 ml) 110 mM Tris in water E ­ Redox agents (yellow, 750 µl) 400 mM GSSG, 200 mM DTT, dissolved in water F ­ Protection

  17. The rotavirus nonstructural protein 4 (NSP4) interacts with both the N- and C- termini of caveolin-1 

    E-Print Network [OSTI]

    Mir, Kiran D

    2006-08-16

    (CSM-Leu-Trp) and then replica plated onto the following selective media: CSM-Leu- Trp-Ura, CSM-Leu-Trp+0.2% 5-Fluoroorotic acid (FOA), and CSM-Leu-Trp-His+3- Aminotriazole (AT) (25mM, 50mM, and 100mM). ?-galactosidase activity was detected...

  18. Successful management of elderly breast cancer patients treated without radiotherapy

    E-Print Network [OSTI]

    Valassiadou, Kalliope; Morgan, David A. L.; Robertson, John F. R.; Pinder, Sarah E.; Cheung, Kwok-Leung

    2007-06-03

    -three cancers were ER positive and 26 were ER negative. ER status was not recorded in four patients. Forty of the 53 ER positive patients were treated with adju- vant tamoxifen. The median size of the cancers was 19 mm (range 2 mm – 40 mm). Seventeen patients...

  19. Examining the Impact of Pad Flexibility on the Rotordynamic Coefficients of Rocker-Pivot-Pad Tilting-Pad Journal Bearings 

    E-Print Network [OSTI]

    Gaines, Jennifer Elizabeth

    2014-12-03

    direction. The measured attitude angles were as high as approximately 10°. The attitude angles remained fairly constant at low rotational speeds for tp = 8.5 mm and tp = 10 mm and decreased as unit load increased for tp = 11.5 mm. XL_TPJB© predicted attitude...

  20. GE PowerPoint Template

    Energy Savers [EERE]

    Type 304 or 316 SS Austenitic, 20% CW, K 25 ksiin, 288C wa ter, NWC 1 x 10 -7 mm s 3 mm year Type 430 17Cr ferritic steel Simila r conditions <1 x 10 -9 mm s 30 m...

  1. Drilling and Microfracture Lead to Different Bone Structure and Necrosis during Bone-Marrow Stimulation for Cartilage Repair

    E-Print Network [OSTI]

    Buschmann, Michael

    Drilling and Microfracture Lead to Different Bone Structure and Necrosis during Bone following microfracture and comparing to drilling in a mature rabbit model of cartilage repair. Microfracture holes were made to a depth of 2 mm and drill holes to either 2 mm or 6 mm under cooled irrigation

  2. The Effects of Variable Quadriceps and Hamstring Loading Configurations on Knee Joint Kinematics During In Vitro Testing

    E-Print Network [OSTI]

    Shalhoub, Sami

    2012-08-31

    configuration of the extensor mechanism, with the largest difference of 2.8° and 0.9 mm at 15° and 45° knee flexion respectively. A weak vastus medialis induced an average lateral shift of 1.5 mm and an external rotation of 0.8° while a 0.9 mm medial shift and 0...

  3. 1 INTRODUCTION 1.1 Jacked piles

    E-Print Network [OSTI]

    Bolton, Malcolm

    the penetration mechanism of a jacked pile to be quantified. Observation of soil adjacent to an advancing pile- trifuge model is discussed. Centrifuge and Constitutive Modelling: Two extremes. Springman S.M. (ed.) pub) De Nicola (1996) Best fit to database of centrifuge tests. L= 150 mm D= 16 mm 0.25­ 0.35 66 mm 6.6 m

  4. Elastic uplift in southeast Greenland due to rapid ice mass loss Shfaqat A. Khan,1

    E-Print Network [OSTI]

    Larson, Kristine

    Elastic uplift in southeast Greenland due to rapid ice mass loss Shfaqat A. Khan,1 John Wahr,2 caused an elastic uplift of $35 mm at a GPS site in Kulusuk. Most of the uplift results from ice dynamic digital elevation models, contributes about $16 mm of the observed uplift, with an additional $5 mm from

  5. Air quality diagnosis from comprehensive observations of total OH reactivity and reactive trace species in urban central Tokyo

    E-Print Network [OSTI]

    2012-01-01

    each instrument through PTFE tubes with a 6.35 mm outsideat 1-min averaging intervals. PTFE tubes with a 6.35 mm o.d.through a 12.7 mm o.d. PTFE tube into a reaction tube by a

  6. Dynamic and Static Characteristics of a Rocker-Pivot, Tilting-Pad Bearing with 50% and 60% Offsets. 

    E-Print Network [OSTI]

    Kulhanek, Chris David

    2012-02-14

    the following characteristics: 5-pads, 101.6 mm (4.0 in) nominal diameter, .0814 - .0837 mm (.0032 - .0033 in) radial bearing clearance, .25 to .27 preload, 60.325 mm (2.375 in) axial pad length. Operating conditions included loads from 0 to 3101 kPa (450 psi...

  7. AN ABSTRACT OF THE THESIS OF Kevin Bradish DelGrande White for the degree of Master of Science in Civil Engineering and

    E-Print Network [OSTI]

    Gupta, Rakesh

    in Civil Engineering and Wood Science presented on March 25, 2005. Title: The Performance of Wood Frame of wood frame shear walls, and more specifically: (1) to compare the performance differences of fully tests were conducted on 2440x2440 mm walls with 38x89 mm Douglas-fir studs 610 mm on center. Two 1220x

  8. Basics of Inertial Confinement Fusion NIF and Photon Science Directorate Chief Scientist

    E-Print Network [OSTI]

    Basics of Inertial Confinement Fusion John Lindl NIF and Photon Science Directorate Chief Scientist - Boston #12;#12;Outline · The challenge of Inertial Confinement Fusion · Development of the science basis to compression in Inertial Confinement Fusion Direct Drive DT gas 2.5 mm 0.1 mm 10 mm #12;The scale of ICF

  9. Management Overview

    Office of Environmental Management (EM)

    0 2 4 6 8 10 12 0 2 4 6 8 10 12 Pu(IV), mM Pu(IV), mM predicted Pu(IV), mM, model Static measurements: Model training database Chemometric model development On-line model...

  10. Experimental Investigations of Properties of Magnetoactive Polymers 

    E-Print Network [OSTI]

    Iyer Ganapathi, Jayadurga

    2012-02-14

    elds were in the order of kV/mm (typically of the order of 0-3 kV/mm to change shear sti ness of 20N/mm)to produce signi cant change in the response [17], [18], [19]. 4. Magnetoactive Smart Polymers Magnetoactive polymers (MAPs) have been developed...

  11. Building Evidence for Active Travel: Counting and Modeling Non-motorized Traffic

    E-Print Network [OSTI]

    Bertini, Robert L.

    Building Evidence for Active Travel: Counting and Modeling Non-motorized Traffic #12;Scope of Talk & maintenance · Test hypotheses and build theory #12;Multi-use Trails in Indianapolis #12;Min Max Mean Week Days B MN* Active Infrared MM MN* Passive infrared P, MM MN MM MN Pressure Pads P P, B? Pneumatic tubes B

  12. Performance Comparison of Nb3Sn Magnets at LBNL

    E-Print Network [OSTI]

    Chiesa, L.

    2011-01-01

    mm) Widtb(mm) Pitch length (mm) RTI RD3b RD3e SMOI III. TESTO! J . ' • • o·~o o 020 RTI SM-O l b - R03~ .. ROll> Iehave been determined for D20, RTI and RD3b, usi ng the coil

  13. (c) 2014 Robert W Heath Jr. WHAT STARTS HERE CHANGES THE WORLD

    E-Print Network [OSTI]

    Heath Jr., - Robert W.

    (c) 2014 Robert W Heath Jr. WHAT STARTS HERE CHANGES THE WORLD Robert W. Heath Jr., Ph.D., P THE WORLD (c) 2014 Robert W Heath Jr. 2 mmWave beamforming mmWave for tactical ad hoc networks mmD students #12;WHAT STARTS HERE CHANGES THE WORLD (c) 2014 Robert W Heath Jr. MIMO precoding Precoding

  14. Rotordynamic evaluation of frequency dependent impedances of hole-pattern gas damper seals 

    E-Print Network [OSTI]

    Holt, Christopher George

    2000-01-01

    Two hole-pattern seals are compared with one smooth bore seal. The two hole-pattern seals have cell depths of 2.03 mm and 3.18 mm with a cell diameter of 1.59 mm. The hole area density factor for both hole-pattern seals is 43%. The L/D ratio...

  15. An Experimental Investigation of the Static and Dynamic Performance of Horizontal-Application and Vertical-Application Three-Lobe Bearings 

    E-Print Network [OSTI]

    Khatri, Rasish

    2014-08-07

    °, 90°, and 100°. This bearing has the following specifications: 100° pad arc angle, 0.52 preload, 70% offset, 101.74 mm (4.0057 in) minimum bore diameter, 0.116 mm (7.55 mils) radial pad clearance, and 76.3 mm (3 in) axial length. The static and dynamic...

  16. Identification with a recombinant antibody of an inner-ear cytokeratin, a marker for

    E-Print Network [OSTI]

    Hudspeth, A. James

    whose expression declines during hair-cell differentiation. Materials and Methods The production were fixed for 1 h at 4°C in 4% (wt vol) formaldehyde in PBS (68 mM NaCl 58 mM Na2HPO4 17 mM NaH2PO4, p

  17. Nucleus Implant Parameters Significantly Change the Compressive

    E-Print Network [OSTI]

    Karduna, Andrew

    stiffness of the denucleated intervertebral disc IVD when im- planted in the created nuclear defect into the custom made molds of three different diameters D1=15 mm, D2=16 mm, and D3=17 mm to achieve variation in the hydrogel implant diameter. The filled molds were gelled by six repeated cycles of freezing for 21 h at -19

  18. > REPLACE THIS LINE WITH YOUR PAPER IDENTIFICATION NUMBER (DOUBLE-CLICK HERE TO EDIT) < 1 Abstract--Compactness and efficiency are the two basic

    E-Print Network [OSTI]

    Mi, Chunting "Chris"

    --Compactness and efficiency are the two basic considerations of the wireless battery chargers for electric vehicles (EVs). At last, a 600mm*600mm with a nominal 150mm-gap wireless charger prototype, operated at a resonant--Electric vehicle (EV), stationary charging, wireless charger, wireless power transfer (WPT), inductive power

  19. UNITED STATES DEPARTMENT OF THE INTERIOR, OSCAR L. CHAPMAN, Secretary FISH AND WILDLIFE SERVICE, ALBERT M. DAY, Director

    E-Print Network [OSTI]

    skipjack, Ka,tsuwonus pelamis. These young fish, measlUwg 35 mm. and 48 mm. in total length,2 were captmed. Yee,3 caught three additional specimens of juveuile K. pelamis. Total lengths of these Bsh were 20 mm of Kats1twon'us pelamis as shown by Kishinouye (1923), Frade and de Buen (1932), and Godsil and Byers

  20. 1 Copyright 2014 by ASME Proceedings of the ASME 2014 33rd International Conference on Ocean, Offshore and Arctic Engineering

    E-Print Network [OSTI]

    Bruneau, Steve

    University of Newfoundland, St. John's, NL, Canada Rocky S. Taylor 1, 2 1 Memorial University of Newfoundland. John's, NL, Canada ABSTRACT A series of small-scale ice indentation tests has been carried out to study indenter shapes (a flat plate and a spherical indenter). Indentation rates of 0.1 mm/s, 1 mm/s and 10 mm

  1. Three new cryptic species of Euglossa from Brazil (Hymenoptera, Apidae)

    E-Print Network [OSTI]

    Nemesio, Andre; Engel, Michael S.

    2012-09-21

    . The metatibia and sterna (Figs 1, 6) are blue, contrasting Figures 1–3. Photomicrographs of paratype male of Euglossa clausi Nemésio and Engel, sp. n. 1 Lateral habitus 2 Dorsal habitus (arrow points to rounded pronotal angle) 3 Facial aspect. Three new...–15). Description. ?: Body length ca. 10.0 mm; forewing length ca. 7.7 mm; head width 4.4 mm; interorbital distance at level of antennal sockets 2.5 mm; maximum interorbital distance 2.7 mm; labiomaxillary complex in repose reaching tip of body; scape length 0...

  2. Random variation in rectal position during radiotherapy for prostate cancer is two to three times greater than that predicted from prostate motion

    E-Print Network [OSTI]

    Scaife, J.; Harrison, K.; Romanchikova, M.; Parker, A.; Sutcliffe, M.; Bond, S.; Thomas, S.; Freeman, S.; Jena, R.; Bates, A.; Burnet, N.

    2014-09-16

    that were less superior on the MV scan were defined as negative. The median difference in position when all days and patients were combined was 3mm, with an IQR of 21.5 to 7.5mm. With an MV slice thickness of 6mm, this meant that the IQR showed ,1 slice... thirds. The range was 21.4 to 4.2 mm for the 10 patients, reflecting S in rectal radius between patients. IQR varied between patients (range, 1.8–6.1mm), corresponding to differences in s be- tween patients. Figure 4. (Supporting material.) Boxplot...

  3. Integrity testing methods for drilled and grouted piles 

    E-Print Network [OSTI]

    Dupin, Richard Martin

    1990-01-01

    . 762 m) and a length of 110 ft (33. 5 m). It had constructed defects in the grout curtain. The insert casing for this pile was 20 in. (0. 508 m) in diameter with a wall thickness of 3/4 in. (19 mm). The other two piles were 8 in. (20. 3 mm...) in diameter and 40 ft (12. 2 m) in length, with a 5 in. (127 mm) diameter, 3/8 in. (9. 5 mm) wall thickness insert casing. One of the two 8 in. (20. 3 mm) diameter piles was constructed with prepared defects while the other one was constructed without...

  4. JBS Crystallization Freshman Kit Junior Cat.-No.: CSK-101 Get a head start crystallizing your protein

    E-Print Network [OSTI]

    Lebendiker, Mario

    Acetate 4.5 200 mM Lithium Sulfate 41 70% v/v MPD None 100 mM HEPES Sodium Salt 7.5 None 42 20% w/v PEG Number Precipitant 1 Precipitant 2 Buffer pH Salt pH 1 50% v/v PEG 400 None 100 mM Sodium Acetate 4.5 200 mM Lithium Sulfate 2 20% w/v PEG 3000 None 100 mM Sodium Citrate 5.5 None 3 20% w/v PEG 3350 None

  5. Euglossa obrima, a new species of orchid bee from Mesoamerica, with notes on the subgenus Dasystilbe Dressler (Hymenoptera, Apidae)

    E-Print Network [OSTI]

    Hinojosa-Dí az, Ismael A.; Melo, Gabriel A. R.; Engel, Michael S.

    2011-10-05

    angles of clypeus); lower clypeal width 2.22 mm (2.19–2.30; n=5) (as measured at level of lower lateral parts); clypeal protuberance 0.76 mm (0.74–0.81; n=5) (following measurement method of Brooks 1988); medial clypeal ridge sharp, paramedial clypeal...; metatibial anterior margin length 3.96 mm (3.78–4.15; n=5), ventral margin length 2.28 mm (2.22–2.44; n=5); postero-dorsal margin length 4.29 mm (4.19–4.52; n=5); metatibial ventro-posterior angle evenly rounded. Forewing length 10.00 mm (9.63– 10.81; n=5...

  6. Plasma Membrane Cholesterol as a Regulator of Human and Rodent P2X7 Receptor Activation and Sensitization

    E-Print Network [OSTI]

    Robinson, Lucy E.; Shridar, Mitesh; Smith, Philip; Murrell-Lagnado, Ruth D.

    2014-10-03

    load- ing on human and mouse P2X7 receptor whole-cell currents and large pore formation. Unlike other P2X receptor subtypes, acute depletion of cholesterol enhanced agonist-evoked cur- rents and membrane permeabilization, whereas cholesterol loading... NES; 149 mM NaCl, 0.8 mM KCl, 0.6 mM CaCl2, 0.08 mM MgCl2, 10 mM D-glucose, 10 mM HEPES, pH 7.3) and imaged using the 40? oil immersion objective on a confocal micro- scope at room temperature. Ethidium bromide (20 ?M in RD NES) and BzATP (300 ?M in RD...

  7. Tubular solid oxide fuel cells with porous metal supports and ceramic interconnections

    DOE Patents [OSTI]

    Huang, Kevin (Export, PA); Ruka, Roswell J. (Pittsburgh, PA)

    2012-05-08

    An intermediate temperature solid oxide fuel cell structure capable of operating at from 600.degree. C. to 800.degree. C. having a very thin porous hollow elongated metallic support tube having a thickness from 0.10 mm to 1.0 mm, preferably 0.10 mm to 0.35 mm, a porosity of from 25 vol. % to 50 vol. % and a tensile strength from 700 GPa to 900 GPa, which metallic tube supports a reduced thickness air electrode having a thickness from 0.010 mm to 0.2 mm, a solid oxide electrolyte, a cermet fuel electrode, a ceramic interconnection and an electrically conductive cell to cell contact layer.

  8. Glutathione Resins I. List of Components

    E-Print Network [OSTI]

    Lebendiker, Mario

    , dilute 4 ml of 10X Extraction/Loading Buffer with 36 ml of deionized water. If necessary, warm is prepacked with 1-ml Glutathione-Uniflow Resin. · 5 x 100 mg of Glutathione (reduced) · 10X Extraction/Loading Buffer (1.4 mM NaCl; 100 mM Na2 HPO4 ; 18 mM KH2 PO4 , pH 7.5): To prepare the extraction/loading buffer

  9. Flow Cell Assays with Microtubules: Motility/Dynamics in Fluorescence and VE-DIC

    E-Print Network [OSTI]

    Mitchison, Tim

    Flow Cell Assays with Microtubules: Motility/Dynamics in Fluorescence and VE-DIC Flow cell assays procedures for flow cell assays. I. Solutions & Supplies BRB80 (1X): 80 mM PIPES, 1 mM MgCl2, 1 mM EGTA, pH 6 below) Flow Cells: Flow cells can be constructed in many different ways. The most common way is to place

  10. Nature Methods Principles for applying optogenetic tools derived from direct

    E-Print Network [OSTI]

    Schnitzer, Mark

    R2 ChR2R ChETAA TC ChETATC CatCh ChIEF FR GR C1V1T C1V1TT Light power density (mW mm-2 ) Light power density (mW mm-2 )Light power density (mW mm-2 ) 60 s light 0 1 2 3 (a) Representative traces representing 5 Successful spikes and plateau potential for injected current-induced and light

  11. SU-E-J-103: Setup Errors Analysis by Cone-Beam CT (CBCT)-Based Imaged-Guided Intensity Modulated Radiotherapy for Esophageal Cancer

    SciTech Connect (OSTI)

    Yang, H; Wang, W; Hu, W; Chen, X; Wang, X; Yu, C [Taizhou Hospital, Wenzhou Medical College, Taizhou, Zhejiang (China)

    2014-06-01

    Purpose: To quantify setup errors by pretreatment kilovolt cone-beam computed tomography(KV-CBCT) scans for middle or distal esophageal carcinoma patients. Methods: Fifty-two consecutive middle or distal esophageal carcinoma patients who underwent IMRT were included this study. A planning CT scan using a big-bore CT simulator was performed in the treatment position and was used as the reference scan for image registration with CBCT. CBCT scans(On-Board Imaging v1. 5 system, Varian Medical Systems) were acquired daily during the first treatment week. A total of 260 CBCT scans was assessed with a registration clip box defined around the PTV-thorax in the reference scan based on(nine CBCTs per patient) bony anatomy using Offline Review software v10.0(Varian Medical Systems). The anterior-posterior(AP), left-right(LR), superiorinferior( SI) corrections were recorded. The systematic and random errors were calculated. The CTV-to-PTV margins in each CBCT frequency was based on the Van Herk formula (2.5?+0.7?). Results: The SD of systematic error (?) was 2.0mm, 2.3mm, 3.8mm in the AP, LR and SI directions, respectively. The average random error (?) was 1.6mm, 2.4mm, 4.1mm in the AP, LR and SI directions, respectively. The CTV-to-PTV safety margin was 6.1mm, 7.5mm, 12.3mm in the AP, LR and SI directions based on van Herk formula. Conclusion: Our data recommend the use of 6 mm, 8mm, and 12 mm for esophageal carcinoma patient setup in AP, LR, SI directions, respectively.

  12. Electromagnetic Tracking of Intrafraction Prostate Displacement in Patients Externally Immobilized in the Prone Position

    SciTech Connect (OSTI)

    Bittner, Nathan [Tacoma/Valley Radiation Oncology Centers, Tacoma, WA (United States); Butler, Wayne M.; Reed, Joshua L.; Murray, Brian C.; Kurko, Brian S. [Schiffler Cancer Center and Wheeling Jesuit University, Wheeling, WV (United States); Wallner, Kent E. [Puget Sound Health Care System, Department of Veterans Affairs, Seattle, WA (United States); Merrick, Gregory S., E-mail: gmerrick@urologicresearchinstitute.or [Schiffler Cancer Center and Wheeling Jesuit University, Wheeling, WV (United States)

    2010-06-01

    Purpose: To evaluate intrafraction prostate displacement among patients immobilized in the prone position using real-time monitoring of implanted radiofrequency transponders. Methods and Materials: The Calypso localization system was used to track prostate motion in patients receiving external beam radiation therapy (XRT) for prostate cancer. All patients were treated in the prone position and immobilized with a thermoplastic immobilization device. Real-time measurement of prostate displacement was recorded for each treatment fraction. These measurements were used to determine the duration and magnitude of displacement along the three directional axes. Results: The calculated centroid of the implanted transponders was offset from the treatment isocenter by >=2 mm, >=3 mm, and >=4 mm for 38.0%, 13.9%, and 4.5% of the time. In the lateral dimension, the centroid was offset from the treatment isocenter by >=2 mm, >=3 mm, and >=4 mm for 2.7%, 0.4%, and 0.06% of the time. In the superior-inferior dimension, the centroid was offset from the treatment isocenter by >=2 mm, >=3 mm, and >=4 mm for 16.1%, 4.7%, and 1.5% of the time, respectively. In the anterior-posterior dimension, the centroid was offset from the treatment isocenter by >=2 mm, >=3 mm, and >=4 mm for 13.4%, 3.0%, and 0.5% of the time. Conclusions: Intrafraction prostate displacement in the prone position is comparable to that in the supine position. For patients with large girth, in whom the supine position may preclude accurate detection of implanted radiofrequency transponders, treatment in the prone position is a suitable alternative.

  13. www.activemotif.comwww.activemotif.com Protein Purification

    E-Print Network [OSTI]

    Lebendiker, Mario

    Storage Resuspension Buffer 45 ml 175 ml Room Temp. Buffer A 33 ml 125 ml Room Temp. Elution Buffer 11 ml. Resuspension Buffer 50 mM Tris, pH 8.0, 300 mM NaCl, and 10 mM Imidazole, 0.2% Triton X-100 2. Lysozyme 100 mg concentration of 0.2% to the Resuspension Buffer. This will help the ly

  14. Oxford University Press 26 October, 2001 All rights reserved. No part of this publication may be reproduced, stored in a retrieval system, or transmitted, in any form or by any means, without the prior

    E-Print Network [OSTI]

    Kirschner, Marc W.

    phosphatase) ¨ 10× CIP buffer (200 mM Tris-HCl, pH 8.0, 10 mM MgCl2, 10 mM ZnCl2) ¨ Water-bath or heating. 4 Purify the phosphatase-treated DNA by phenol extraction and ethanol precipitation (see.0, or water. 5 Because of the stability of the enzyme and the consequences of its persistence in subsequent

  15. About the university Virginia Commonwealth University

    E-Print Network [OSTI]

    Motai, Yuichi

    backgrounds can thrive. mechanical-and-nuclear.egr.vcu.edu gradmne@vcu.edu 0.570 0.840 0.0984 0.178 12mm 0.0625" R 3.1mm 2.0 mm 0.295 0.456 0 0.295 0.570 0.178 0.100 0 Mechanical and Nuclear Engineering Mechanical Engineering is, therefore, one of the oldest and broadest of the engineering disciplines. Nuclear Engineering

  16. Development of a General-purpose Expandable Arm for a Small Mobile Robot Tatsuya HASHIMOTO, University of Tsukuba

    E-Print Network [OSTI]

    Ohya, Akihisa

    ; a rotary degree of freedom at the base, a stretching degree of freedom and a rotary degree of freedom in the stretching section, DC motors for driving, Harmonic-drive to reduce the speed and a solenoid to push switches, Harmonic-drive, Solenoid 1. 1)2) 2. 2·1 2·1.1 · 3) · 2·1.2 2·2 370mm 322mm 420mm 2·3 40cm #12;88cm Fig.1

  17. New Measurements of the Radio Photosphere of Mira based on Data from the JVLA and ALMA

    E-Print Network [OSTI]

    Matthews, L D; Menten, K M

    2015-01-01

    We present new measurements of the millimeter wavelength continuum emission from the long period variable Mira ($o$ Ceti) at frequencies of 46 GHz, 96 GHz, and 229 GHz ($\\lambda$~7 mm, 3 mm, and 1 mm) based on observations obtained with the Jansky Very Large Array (JVLA) and the Atacama Large Millimeter/submillimeter Array (ALMA). The measured millimeter flux densities are consistent with a radio photosphere model derived from previous observations, where flux density, $S_{\

  18. Flat Beam Generation Kwang-Je Kim

    E-Print Network [OSTI]

    Flat Beam Generation Kwang-Je Kim Argonne National Laboratory and The University of Chicago 26th-6, 2002 #12;Flat Beam Generation Beam adapter: Ya. Derbenev Theory: A. Burov, S. Nagaitsev, Ya. Derbenev Colliders TESLA NLC CLIC Q (nc) 3 1.6 0.6 x (mm-mrad) 12 4.5 0.68 y (mm-mrad) 0.03 0.1 0.02 (mm-mrad) 0.6 0

  19. Testing of hollow clay tile masonry prisms

    SciTech Connect (OSTI)

    Jones, W.D.; Butala, M.B.

    1993-10-15

    This paper presents test results of 610-mm wide (24-in.) by 1219-mm high (48-in.) by 203-or 330-mm (8- or 13-in.) thick prisms constructed of hollow clay tiles. Three prisms were extracted fro existing hollow clay title walls and 69 were constructed in laboratories at The University of Tennessee and the National Institute of Standards and Technology (NIST) in Gaithersburg, Maryland. Modulus of Elasticity, E, and compressive strength f{prime}{sub m} were calculated from the results.

  20. AN ABSTRACT OF THE THESIS OF Peter Seaders for the degree of Master of Science in Civil Engineering and Wood Science

    E-Print Network [OSTI]

    Gupta, Rakesh

    and Wood Science presented on September 24, 2004. Title: Performance of Partially and Fully Anchored Wood. Miller The objectives of this study were to evaluate the performance of wood frame shear walls under specimens with 38 x 89 mm (2x4) Douglas-fir studs at 610 mm (24 in) on center. Two 1220x2440x11.1 mm (48x96x